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Astrophysics of galaxies
The materials of the exhibition cover a wide range of issues related to the study of galaxies and intergalactic space. The publications presented at the exhibition introduce the composition, structure and development of stellar systems, the evolution of the interstellar medium, galaxies and galaxy clusters. The publications consider the physical, chemical and dynamic processes occurring in the interstellar medium, present the results of studies of gas movements in interstellar space and in stellar atmospheres, give a brief overview of modern ideas about the interplanetary dust cloud, describe the features of galaxies, as well as the evolution of views on their origin.
During the preparation of the exhibition, publications from the fund of the Russian National Public Library for Science and Technology were used: monographs, collections of scientific papers, textbooks and manuals, conference materials, articles from specialized journals, abstracts of dissertations, preprints, publications from the electronic library systems "Lan", "ZNANIUM.COM ", IPR SMART digital educational resource, database of Russian publications of the company East View Information Services, as well as publications from the Springer publishing house's full-text database.
The materials of the exhibition may be of interest to researchers – astronomers and physicists interested in astrophysics and dynamics of stellar systems, graduate students, senior physics students, teachers.
The materials of the exhibition can be found in the lobby of the 2nd floor of the main building from June 8 to August 18, 2022. At the end of the exhibition period, you can pre-order the print edition you are interested in from the list by clicking the "ORDER" button. To order, authorization is required in the reader's Personal Account. You can work with publications in the reading room selected by you when placing an order.
If you have any questions about the use of printed publications presented at the exhibition, please call: 8(495) 698-93-07, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it. or in a chat on the main page of the library's website.
Authorization is required to read electronic publications presented at the exhibition. The terms of access can be found in your Personal Account in the section "Licensed resources".
Thematic sections of the exhibition:
2. Physics of the interstellar medium
1. Д10-16/31540
Аккреционные процессы в астрофизике / П. К. Аболмасов [и др.] ; под редакцией Н. И. Шакуры. – Москва : Физматлит, 2016. – 416 с. : ил. – Авт. указ. на обороте тит. л. – Библиогр. в конце гл. – ISBN 978-5-9221-1633-6. – Текст : непосредственный.
Abstract: The fundamentals of the modern theory of disk and quasi-spherical accretion on black holes and magnetized neutron stars are presented. Relativistic corrections near the inner radius of the disk are calculated. The dynamics of bending disks around rotating black holes is considered. The structure of accretion disks around supermassive black holes in active galactic nuclei is studied. The theory of transient growth of perturbations in Keplerian disks is considered. Some aspects of the development of magneto-rotational instability in disks are discussed. The visco-convective instability in thin laminar Keplerian disks, which can initiate the development of turbulence, is considered. The book is intended for senior students, graduate students and specialists in the field of high-energy astrophysics.
2. Д8-98/40413
Актуальные проблемы внегалактической астрономии : ХV конференция, 25-29 мая 1998 г. : программа и тезисы докладов / Пущинская радиоастрономическая обсерватория. – Пущино : [б. и.], 1998. – 59 с. – В надзаг. : Пущинc. Радиоастроном. обсерватория АКЦ ФИАН, Астроном. ин-т С.-Петерб. ун-та, Рос. фонд фундамент. исслед., Радиоастроном. учеб.-науч. центр. – Текст : непосредственный.
Abstract: This collection contains abstracts of reports submitted to the XV Annual Conference on Extragalactic Astronomy, organized by the Pushchina Radio Astronomy Observatory of the ACC FIAN together with the Astronomical Institute of St. Petersburg University. The topics of the conference cover a wide range of problems of extragalactic astronomy and include reports on the results of observations of extragalactic objects in various electromagnetic wave ranges, as well as theoretical papers dealing with the problems of active galaxies, the large-scale structure of the Universe and cosmology.
3. Д8-02/82629
Бааде, В. Эволюция звезд и галактик : курс лекций / В. Бааде ; перевод с английского Ю. Н. Ефремова ; под редакцией А. С. Шарова. – 2-е изд., стереотип. – Москва : УРСС, 2002. – 299 с. : ил. – Пер.изд.: Baade W. Evolution of stars and galaxies. – Cambrige, 1963. – ISBN 5-354-00188-9. – Текст : непосредственный.
Abstract: The book is a course of lectures delivered by V. Baade to students of Harvard University and employees of the Harvard Observatory (USA). The topic of the lectures is the properties and evolutionary development of stars and giant star systems – galaxies. The author of the book is the creator of modern ideas about the composition and structure of stellar systems. He worked for many years on the largest telescopes in the world, gained a lot of experience in this and collected a wealth of observational material about stars of various types and the structure of galaxies. In his lectures, the author made extensive use of the results he obtained; some of them have not yet been published by him, and this gives the book special value. The book is written at a high scientific level and at the same time in a fairly simple language. It will be useful for both astronomers and students, as well as readers who are seriously interested in astronomy, especially physicists dealing with problems of astrophysics and cosmology.
4. Д10-17/40792
Галактики / В. С. Аведисова [и др.] ; редактор-составитель В. Г. Сурдин. – 2-е изд., испр. и доп. – Москва : Физматлит, 2017. – 431 с. : ил. – Авт. указ. на обороте тит. л. – ISBN 978-5-9221-1726-5. – Текст : непосредственный.
Abstract: The fourth book in the series "Astronomy and Astrophysics" contains an overview of modern ideas about giant star systems – galaxies. It tells about the history of the discovery of galaxies, their main types and classification systems. The fundamentals of the dynamics of stellar systems are given. The galactic surroundings closest to us and the work on the global study of the Galaxy are described in detail. Data on various types of galaxy populations – stars, interstellar medium and dark matter are presented. The features of active galaxies and quasars are described, as well as the evolution of views on the origin of galaxies. The book is aimed at undergraduate students of natural science faculties of universities and specialists in related fields of science. The book is of particular interest to fans of astronomy.
5. М/42146/106-СПб
Госачинский, И. В. Структура слоя газа во внешних спиральных рукавах первого квадранта галактических долгот / И. В. Госачинский, В. О. Дмитриев. – Санкт-Петербург : [б. и.], 1995. – 12 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 106-СПб)). – Текст : непосредственный.
Abstract: The z-coordinate structure of the gas was studied in the first quadrant of galactic longitudes for three outer spiral arms according to the HI survey on RATAN-600. The layer parameters (thickness and z-coordinate of the center of gravity) were determined separately for the "wide" and "narrow" components of the layer. The parameters of "folding" are obtained – along and across the sleeves.
6. Д10-15/20606
Гречкосей, Е. Н. Черная дыра. Квазар. Светящаяся галактика / Е. Н. Гречкосей. – Санкт-Петербург : Периферия, 2015. – 79 с. : ил. – Библиогр.: с. 79 (2 назв.). – ISBN 978-5-906168-08-5. – Текст : непосредственный.
Abstract: The book describes the process that occurs with each galaxy at all stages of its evolutionary cycle. A new discovery is the description of the transition of the galaxy from the state of a "black hole" to the state of a quasar. The proposed model organically fits into the general model of S. A. Nikolaev's cosmological theory "The Universe of Different Ages". In addition, this model of the transition of a "black hole" into a quasar state explained a lot of unresolved issues arising from astronomical observations. The book is intended for a wide range of people with secondary and higher education, as well as students of secondary and higher educational institutions interested in the problems of matter and the Universe.
7. Ар18-5455
Гусев, А. С. Звездное население и процессы современного звёздообразования в галактиках : специальность 01.03.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / А. С. Гусев ; Московский государственный университет имени М. В. Ломоносова. – Москва, 2018. – 31 с. – Библиогр.: с. 16-21 (36 назв.). – Текст : непосредственный.
8. Данилов, В. М. Нестационарность рассеянных звездных скоплений : монография / В. М. Данилов. – Екатеринбург : Уральский федеральный университет, ЭБС АСВ, 2015. – 484 c. – ISBN 978-5-7996-1636-6 // Цифровой образовательный ресурс IPR SMART : [сайт]. – URL: https://www.iprbookshop.ru/66557.html (дата обращения: 27.04.2022). – Access mode: for authorization. users. – Text : electronic.
Abstract: The monograph consistently presents issues related to the study of the nonstationarity of scattered star clusters, starting with the analysis of the properties of the trajectories of single stars to the analysis of collective movements of stars, discussing the dynamics of correlations and wave processes in such clusters. The astrophysical applications of the results of studying the dynamics of the RSL are considered. The book contains formulas, tables, figures and can be used for research work in the field of dynamics of stellar systems. For researchers – astronomers and physicists interested in astrophysics and dynamics of stellar systems, graduate students and undergraduates of relevant specialties.
9. М/42146/106 СПб
Дравских, А. Ф. Квазары, входящие в ассоциации с галактиками / А. Ф. Дравских, З. В. Дравских. – Санкт-Петербург : [б. и.], 1994. – 19 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 106 СПб)). – Текст : непосредственный.
Abstract: The results of statistical comparison of quasars associated with galaxies and quasars with absorption spectra are presented. Based on the data obtained, the hypothesis previously put forward by the authors about the genetic relationship of quasars and galaxies is clarified. An experimental test of the hypothesis is proposed.
10. М/42146/118
Дравских, А. Ф. Квазары с абсорбциями как центры крупномасштабных неоднородностей квазаров во вселенной / А. Ф. Дравских, З. В. Дравских. – Санкт-Петербург : [б. и.], 1996. – 27 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 118). – Текст : непосредственный.
Abstract: This paper presents relative statistical studies of the three-dimensional spatial distribution of ~ 7 thousand quasars of the modern catalog. The result is obtained, which shows that if we remain in the positions of the standard Friedman cosmological model of the universe, then quasars with absorptions are the centers of large-scale (1000 megaparsecs or more) inhomogeneities in the spatial distribution of quasars. Inhomogeneities look like a shortage of quasars around quasars with removals. The density of quasars around these centers is reduced to 3 times relative to their density around quasars without absorption.
11. М/42146/142
Дравских, А. Ф. Оценка эволюции размеров газовой составляющей галактик и облаков газа на интервале Z от О до 3.6 / А. Ф. Дравских. – Санкт-Петербург : [б. и.], 2003. – 15 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Ленинград) ; 142). – Библиогр.: с. 15 (11 назв.). – Текст : непосредственный.
Abstract: It is shown that the absorbers observed in the absorption spectra of quasars can be used to study the evolution of the size of the gas component of galaxies and gas clouds at large z intervals. The evolution of the linear dimensions L of these objects in the range z from ~0 to 3.6 was estimated. A total of 265 quasars in the range z from 0.288 to 3.803 and 809 absorbers associated with them in the range z from ~0 to 3.5575 were used. The estimate L = L 0(1 + z) 1.73±0.07 was obtained.
12. М/42146/119
Дравских, А. Ф. Центры крупномасштабных неоднородностей распределения квазаров во Вселенной / А. Ф. Дравских, Д. А. Дравских. – Санкт-Петербург : [б. и.], 1997. – 13 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 119). – Текст : непосредственный.
Abstract: Statistical studies of the catalog of quasars containing more than 7 thousand objects have shown that quasars associated with galaxies have spatial distribution features similar to those of quasars with absorptions.
13. Ар14-13591
Ермаш, А. А. Сейфертовские галактики первого типа с узкими линиями – активные ядра в спиральных галактиках с псевдобалджами : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Ермаш А. А. – Москва, 2014. – 24 с. : ил. – Библиогр.: с. 21 (40 назв.). – Текст : непосредственный.
14. Закутняя, О. Рентгеновские тайны галактики / Ольга Закутняя. – Text : electronic // Наука и жизнь. – 2009. – №7. – С. 2-4. – URL: https://dlib.eastview.com/browse/doc/20476133 (дата обращения 11.04.2022). – Access mode: for authorization. users.
Abstract: The mysterious glow of the Galaxy's disk in X-rays, discovered more than 25 years ago, has finally found its explanation. A group of astrophysicists from the Institute of Space Research of the Russian Academy of Sciences (IKI RAS), led by Mikhail Revnivtsev, experimentally showed that the X–ray radiation of the disk of our Galaxy consists of the emissions of millions of weak sources - mainly so-called white dwarfs and stars with active corona.
15. М/14715/1409
Зенцова, А. С. О взаимосвязи оптического и радиоизлучения ядер активных галактик и квазаров / А. С. Зенцова, В. Н. Федоренко. – Ленинград, 1989. – 20 с. : ил. – (Препринт / Физико-техн. ин-т им. А. Ф. Иоффе (Ленинград); 1409). – Библиогр.: с. 19 (26 назв.). – Текст : непосредственный.
Abstract: A model has been developed according to which the radio emission of compact extragalactic sources (Seyfert galaxies, quasars) occurs in the regions of formation of their wide optical lines RB~1018-1019 cm. The latter are assumed to consist of a large number (Nc~106) of dense clouds (nc~1010 cm-3) flying radially at velocities Uc~108÷109 cm/s. The clouds are immersed in a hot (Tw~107K), sparse (nw~107 cm3) wind, also radially scattering at a speed of Uw~109 cm/s. The relative motion of clouds and wind is considered supersonic. In the regions of shock waves, electrons are accelerated to relativistic energies. These electrons form radial tracks behind clouds, similar to the tails of comets, and create the observed synchrotron radiation in the presence of magnetic fields in the regions under consideration.
16. М/42146/116
Исследование галактик в площадке неба по прямому восхождению 2 16 – 2 40 и по склонению от – 3 до – 8 40 / А. Серрано, А. А. Липовка, О. Кардона и др. – Санкт-Петербург : [б. и.], 1996. – 15 c. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 116). – Текст : непосредственный.
Abstract: A catalog of galaxies up to 21m in an almost unexplored area of 16.25 square degrees is proposed. The proportion of blue galaxies in the present sample is several times greater than it follows from the morphological type– density ratio of galaxies for the nearest clusters, and is more than 50% of the total number of galaxies.
17. М/42146/126
Исследование галактик в скоплении А1185 и его окрестностях / А. М. Боташев, О. В. Верходанов, О. Кардона [и др.]. – Санкт-Петербург : [б. и.], 1997. – 21 с. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 126). – Текст : непосредственный.
Abstract: The results of the study of a close cluster of A1185 galaxies in the optical, radio and submillimeter wave ranges are presented. The coordinates of 115 cluster members and field galaxies located in this cluster are obtained. Radio observations were carried out on RATAN-600 on waves 2.7, 3.9, 7.6, 13 and 31 cm. Using our data and data published by other authors, we obtained the oadiospectrs of a number of galaxies in the A1185 cluster.
18. М/42146/130 СПб
Исследование области неба с обилием голубых галактик / О. В. Верходанов, О. Кардона, Н. М. Липовка [и др.]. – Санкт-Петербург : [б. и.], 1999. – 13 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 130 СПб). – Текст : непосредственный.
Abstract: The work continues the studies of galaxy clusters, the catalog of which was previously published (Serrano et al. 1996). Radio emission at a frequency of 1400 MHz was detected from more than 10% of the objects, and 70% of them are active galaxies with an excess of color in blue rays.
19. М/9354/66(1999)
Кардашев, Н. С. Два типа квазаров и пульсаров / Н. С. Кардашев. – Москва, 1999. – 13 с. – (Препринт / Физический ин-т им. П. Н. Лебедева (Москва) ; 66 (1999)). – Текст : непосредственный.
Abstract: The possibility of synchrotron radiation of extremely high intensity in the magnetospheres of supermassive black holes and neutron stars by relativistic protons is investigated. The main parameters of such a model are determined. The possibility of existence of two types of objects is shown, one with acceleration and emission of relativistic protons, the other – relativistic electrons.
20. М/42146/132
Каталог ярких галактик в окрестности скопления А569 / Н. М. Липовка, А. А. Липовка, Е. Чавира, О. В. Верходанов. – Санкт-Петербург : [б. и.], 1999. – 17 с. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 132). – Текст : непосредственный.
Abstract: This paper presents a catalog of 217 galaxies up to 18ɱ located in the direction of the A569 cluster.The coordinates of the galaxies were obtained in Tonatsintla (Mexico). This area of the sky is of particular interest, since there are at least three more subclusters in the vicinity of A569, which are probably gravitationally bound.
21. М/42146/140
Каталог ярких галактик и диффузных объектов в скоплении А2151 / Е. Чавира, О. Кардона, Н. М. Липовка, А. А. Липовка. – Санкт-Петербург : [б. и.], 2002. – 16 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 140). – Текст : непосредственный.
Abstract: In this paper, the A2151 galaxy cluster located at Z=0.031-0.041 is investigated. A catalog of 75 bright cluster members whose coordinates were calculated using a blink comparator from copies of the Palomar Glass Library at the National Institute of Astronomy, Optics and Electronics (INAOE, Mexico) is given.
22. М/46033/48(1990)
Кац, А. В. Функция светимости квазаров в модели слияний / А. В. Кац, В. М. Конторович. – Харьков, 1990. – 19 с. – (Препринт ; 48 (1990)). – Библиогр.: с. 18-19 (18 назв.). – Текст : непосредственный.
Abstract: The luminosity function of active galactic nuclei (quasars) is calculated under the assumption that the cause of activity is accretion to a compact object in the core, and the cause of accretion is compensation of the moment during the merger of spiral galaxies within the framework of the phenomenological model proposed by the authors.
23. М/9354/31(2011)
Комберг, Б. В. Морфология и эволюционный статус активных галактик типа NLSy 1 / Б. В. Комберг, А. А. Ермаш. – Москва, 2011. – 53 с. : ил. – (Препринт / Физический ин-т им. П. Н. Лебедева (Москва) ; 31). – Библиогр.: с. 47-52 (99 назв.). – Текст : непосредственный.
Abstract: This work is a review of publications devoted to active galaxies of the NLS type. The NLS objects are considered as a set of many structures, processes and factors, such as: location in a large-scale structure, morphology of the parent galaxy both on a large scale and in the near-nuclear region, structure of BLR (areas of formation of wide lines) and NLR (areas of formation of narrow lines), accretion disk, jets, near-nuclear outflows, rotation of a supermassive black hole, etc. Special attention is paid to current ideas about the evolutionary status of objects of this type.
24. Ар17-2651
Кравченко, Е. В. Многочастотные поляриметрические исследования физических условий в активных ядрах галактик : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Кравченко Е. В. – Москва, 2017. – 24 с. – Библиогр.: с. 21-24 (48 назв.). – Текст : непосредственный.
25. Ар11-6934
Курбатов, Е. П. Численное моделирование химической эволюции галактик : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Курбатов Е. П. – Москва, 2011. – 17 с. : ил. – Библиогр.: с. 12-16. – Текст : непосредственный.
26. Д10-12/37972
Кутузов, С. А. Математические методы моделирования галактик / С. А. Кутузов, М. А. Марданова, Л. П. Осипков ; Санкт-Петербуржский государственный университет, Факультет прикладной математики – процессов управления. – Санкт-Петербург : Соло, 2012. – 114 с. : ил. – Библиогр. в конце гл. – ISBN 978-5-98340-266-9. – Текст : непосредственный.
Abstract: This publication discusses mathematical methods for constructing models of stellar systems; discusses hydrodynamic models of the Galaxy, methods of photometric modeling of galaxies and some fundamental issues of galaxy dynamics. The book is intended for undergraduates and postgraduates who apply methods of applied mathematics in their work, as well as in problems of modeling space systems.
27. Ар15-14021
Лыскова, Н. С. Методы определения масс эллиптических галактик, применимые для больших обзоров : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Лыскова Н. С. – Москва, 2015. – 16 с. : ил. – Библиогр.: с. 14-16. – Текст : непосредственный.
28. Ар17-8627
Медведев, П. С. Физические процессы в горячей астрофизической плазме: диффузия элементов в межгалактической и межзвёздной среде, рентгеновское излучение джетов микроквазаров : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Медведев П. С. – Москва, 2017. – 16 с. : ил. – Библиогр.: с. 15-16. – Текст : непосредственный.
29. Ар11-4874
Мельник, А. М. Кинематика внешних псевдоколец и спиральная структура Галактики : специальность 01.03.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Мельник А. М. – Москва, 2011. – 26 с. – В надзаг.: МГУ им. М. В. Ломоносова, Гос. астроном. ин-т им. П. К. Штернберга. – Библиогр.: с. 22-26 (59 назв.). – Текст : непосредственный.
30. Д9-05/10775
Морозов, А. Г. Физика дисков / А. Г. Морозов, А. В. Хоперсков. – Волгоград : Изд-во ВолГУ, 2005. – 422 с. : ил. – (Труды ученых ВолГУ). – Библиогр.: с. 381-422 (912 назв.). – ISBN 5-9669-0014-0. – В надзаг.: Волгогр. гос. ун-т. – Текст : непосредственный.
Abstract: The book discusses the physical processes that determine the dynamics and spatial structure of astrophysical disks (stellar and gas disks of galaxies, accretion disks around compact objects, in protostellar and protoplanetary systems). A consistent study of the dynamics of small disturbances and stability issues for collisionless and gas-dynamic systems is carried out. The physics of numerous instabilities is considered in detail. The main nonlinear results based on numerical (computer) experiments are presented. Some mechanisms of formation of the spiral structure of galaxies are discussed. It is intended for researchers, postgraduates and undergraduates.
31. Ар11-5429
Москвитин, А. С. Спектроскопический и фотометрический мониторинг массивных сверхновых и послесвечений гамма-всплесков : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Москвитин А. С. – Нижний Архыз, 2011. – 15 с. – В надзаг.: Рос. АН, Спец. астроном. обсерватория. – Библиогр.: с. 6-9. – Текст : непосредственный.
32. М/42146/131 СПб
О возможности использовать данные многоцветной фотометрии для оценки красного смещения далеких радиогалактик и возраста звездных систем их родительских галактик (приложение к препринту N 129 СПб) / О. И. Верходанов, А. И. Копылов, Ю. Н. Парийский [и др.]. – Санкт-Петербург : [б. и.], 1999. – 63 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 131 СПб). – Текст : непосредственный.
Abstract: The results of calculations of redshifts and ages for 49 objects are presented in a visual form on the redshift-age plane of star systems.
33. Ар20-5489
Опарин, Д. В. Изучение воздействия звездообразования на ионизованный газ в галактиках : специальность 01.03.02 – Астрофизика и звёздная астрономия : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Опарин Дмитрий Владимирович ; Специальная астрофизическая обсерватория Российской академии наук. – Нижний Архыз, 2020. – 15 с. – Библиогр.: с. 13-15 (24 назв.). – Текст : непосредственный.
34. Р1968
Письма в Журнал экспериментальной и теоретической физики / Институт физических проблем имени П. Л. Капицы, Российская академия наук. – Москва : Наука, 1965 – (Москва). – Перевод заглавия: Letters to the «Journal of Experimental and Theoretical Physics». – Журнал изд. МАИК «Наука / Интерпериодика» на англ. яз. – До 2005 г. надзаг.: РАН. Отделение общей физики и астрономии. – До 2005 г. период. : ежемесячно. – Журн. изд. под рук. Отд-ния физ. наук РАН. – До 2019 г. изд-во : Наука. – Выходит дважды в месяц. – ISSN 0370-274X. – Текст : непосредственный.
35. Понятов, А. Долгожданное признание черных дыр / Алексей Понятов. – Text : electronic // Наука и жизнь. – 2019. – №11. – С. 24-33. – URL: https://dlib.eastview.com/browse/doc/62293698 (дата обращения 11.04.2022). – Access mode: for authorization. users.
Abstract: This year, the awarding of the Nobel Prize in Physics turned out to be unusual: the Nobel Committee violated two of its long-standing rules at once. The first of them is not to give an award to representatives of one direction in physics for two years in a row. Since the field of physical research has become very wide, and there are quite a lot of researchers working at the Nobel level, this allows us to give an award to scientists from different branches of physics. But in 2020, as in the previous year, the prize was awarded for space exploration. Moreover, the prize was given for the discovery of black holes, some properties of which are still debatable - and this is the second deviation from the rules, since it is customary to award an award for reliably established discoveries. What made the conservative Nobel Committee do this? In my opinion, two factors contributed to this. First, in 2019, the first ever image of a black hole in the galaxy M 87 was obtained. Such a huge achievement of modern astronomy, which has become a direct proof of the existence of these exotic objects, itself deserves the Nobel Prize. Together with the discovery in 2015 of gravitational waves from the merger of black holes, it turned black holes from hypothetical objects into real ones, making it possible to award a prize for their research. But the second possible factor that predetermined the award of the prize "out of turn", namely in 2020, is the desire to have time to award at least one of the remarkable galaxy of physicists of the 1950s and 1960s, who laid the foundations of the theory of black holes. Stephen Hawking (1942-2018) recently passed away and only Roger Penrose, who turned 89 this year, remained alive. It can be said that in his person all this direction of astrophysics received an award. For the sake of this, the Nobel Committee went to award the prize for theoretical, essentially mathematical work, the main provisions of which – the presence of an event horizon and a singularity in a black hole – still remain, strictly speaking, experimentally unproven, although, of course, indirect evidence is available.
36. Понятов, А. Пульсирующая / А. Понятов. – Text : electronic // Наука и жизнь. – 2018. – №6. – С. 36-46. – URL: https://dlib.eastview.com/browse/doc/51364548 (дата обращения 11.04.2022). – Access mode: for authorization. users.
Abstract: Cepheids – huge, like breathing stars, with a surface that rises and starts under the action of internal forces – got their name in honor of the heroine of our story – δ (delta) Cepheus. Perhaps there are no objects in space more caressed by the attention of astronomers than these pulsating and changing stars. Cepheids played a key role in the revolution of our ideas about the universe at the beginning of the twentieth century and became a powerful tool for its research. The lighthouses of the universe, as they are often called, continue to lead the ship of science to new shores of knowledge to this day.
37. Поройков, С. Ю. Вклад дрейфующих нейтронных звезд, ускоренных взрывами сверхновых в протогалактиках во взаимной отталкивание галактик / С. Ю. Поройков. – Text : electronic // Журнал естественнонаучных исследований. – 2019. – № 3. – С. 20-52. – URL: https://znanium.com/catalog/product/1066491 (дата обращения: 27.04.2022). – Access mode: for authorization. users.
Abstract: It is shown that supernova explosions can accelerate pulsars to a velocity of ≤ 1600 km/s. Neutron stars accelerated by supernova explosions can drift towards the corona of galaxies, replenishing their hidden mass, as well as filling intergalactic space. It is shown that drifting metagalactic neutron stars, skirting the surrounding galaxies in hyperbolic orbits, can contribute to their mutual repulsion in the conditions of the observed homogeneous large-scale distribution of the matter of the Universe. At the same time, neutron stars, whose mass corresponds to the mass of the so-called dark energy, could be generated and accelerated by supernova explosions in proto-galaxies.
38. Поройков, С. Ю. Расширение войдов и их субструктур под давлением космических лучей, рассеиваемых магнитным полем гало (корон) галактик / С. Ю. Поройков. – Text : electronic // Журнал естественнонаучных исследований. – 2021. – № 4. – С. 15-30. – URL: https://znanium.com/catalog/product/1860798 (дата обращения: 27.04.2022). – Access mode: for authorization. users.
Abstract: It is shown that the gravity of matter in the voids will be balanced by the pressure on the corona of galaxies in filaments of metagalactic cosmic rays (CL) with an energy density of ~0.1 eV/cm3, which can be scattered by the magnetic field of the corona of galaxies ~4 mcGs with an energy density of ~ 0.3 eV/cm3, formed by relativistic objects in binary systems. The source of CL can be objects with active nuclei with an energy release per one typical galaxy of ~5×1043 erg/s. Waters with a radius of ~20 Mpc contain ultra diffuse galaxies (UDC) of low surface brightness, having an extended massive dark halo. UDGs form spherical substructures with a radius of ~2 Mpc in the waters. Substructures in the waters can be formed by the pressure of metagalactic CL scattered by the magnetic field of the halo of the UDG with a radius of ~ 100 kpc, comparable to the radius of the corona of the galaxies of the general population.
39. М/42146/121
Проблема радиоселекции далеких галактик во Вселенной (положение на 1996 год) / Ю. Н. Парийский, Н. С. Соболева, А. В. Темирова, О. В. Верходанов. – Санкт-Петербург : [б. и.], 1997. – 63 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 121). – Текст : непосредственный.
Abstract: The information obtained in recent years on 193 distant galaxies with redshift >1 by the method of radioselection according to published data is presented. The statistical relationships between the various parameters of these objects in the optical and radio ranges are clarified.
40. Ар15-6126
Пушкарев, А. Б. Коллимированные выбросы вещества в активных ядрах Галактик : специальность 01.03.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Пушкарев А. Б. – Санкт-Петербург, 2015. – 30 с. : ил. – Библиогр.: с. 22-30. – Текст : непосредственный.
41. М/47368/158
Пятунина, Т. Б. Эволюционные закономерности в вариациях потоков, спектров и структуры избранных блазаров / Т. Б. Пятунина, Д. К. Габузда, С. Г. Марченко-Эрштад. – Санкт-Петербург, 2004. – 36 с. : ил. – (Препринт / Институт прикладной астрономии (Ленинград) ; 158). – Библиогр.: с. 31-36(60 назв.). – Текст : непосредственный.
Abstract: The results of studies of the variability of blazars according to RSDB observations at frequencies of 8 and 43 GHz, as well as monitoring in the range (4.8-37) GHz are presented. Time series analysis of selected bazaars reveals quasi-periodic variations of flows with characteristic times from 1 year to 13 years. The evolution of the structure of blazars indicates that short-periodic variations of flows with scales of (1-4) years are due to the evolution of the jet and can be explained, for example, by the evolution of individual clumps, jet precession, or the development of a shock wave system inside the jet, creating successive rarefactions and compressions. Variations with characteristic times of 4 years or more are probably associated with the global evolution of the source, and in some cases, with the cyclical nature of its activity. A typical scenario of the activity cycle is discussed, based on a comprehensive analysis of the variations of the fluxes, spectra and structure of these blazars.
42. Д10-21/88657
Рыбкин, В. В. Электричество и магнетизм космических тел / В. В. Рыбкин. – Москва : Евроазиатская научно-промышленная палата, 2021. – 409 с. : ил. – Библиогр.: с. 397-403 (184 назв.). – ISBN 978-5-6044482-6-7. – DOI 10.17513/пр.444. – Текст : непосредственный.
Abstract: The book presents the results of theoretical research based on a new physical phenomenon predicted by the author – quantum energy losses in matter waves (de Broglie waves). These losses are expressed in the fact that any moving particle becomes a source of weak low-frequency electromagnetic radiation. The radiation flux is directed forward along the trajectory of the particle and is accompanied by a decrease in its momentum. It is shown that this is consistent with observations of small mechanical effects that occur during the movement of Solar system bodies. For a rotating body, the intensity vector of the electric field of radiation has vortex and non-vortex components. The vortex component of the electric field leads to the appearance of an annular current inside the rotating cosmic bodies of the coaxial axis of rotation and the dipole magnetic field caused by it. The electric field generated inside and outside the rotating cosmic body creates large potential differences.
43. Ар09-2817
Рябинков, А. И. Пространственно-временное распределение абсорбционных систем в спектрах квазаров : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Рябинков А. И. – Санкт-Петербург, 2008. – 18 с. – Библиогр.: с. 17-18. – Текст : непосредственный.
44. Ар06-13604
Сазонов, С. Ю. Взаимодействие реликтового излучения, рентгеновского излучения квазаров и ядер активных галактик с межгалактическим и межзвездным газом : специальность 01.03.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Сазонов С. Ю. – Москва, 2006. – 23 с. : ил. – Библиогр.: с. 21-23 (25 назв.). – Текст : непосредственный.
45. Ар16-5930
Свинкин, Д. С. Наблюдения коротких гамма-всплесков в эксперименте Конус-Винд : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Свинкин Д. С. – Санкт-Петербург, 2016. – 18 с. : ил. – Библиогр.: с. 17-18. – Текст : непосредственный.
46. Д10-17/40556
Сильченко, О. К. Происхождение и эволюция галактик / О. К. Сильченко ; под редакцией В. Г. Сурдина. – Фрязино : Век 2, 2017. – 223 с. : ил. – ISBN 978-5-85099-196-8. – Текст : непосредственный.
Abstract: The book presents the current state of our knowledge and the author's personal ideas about the formation and evolution of galaxies in the universe. Galaxies–large formations consisting of billions of stars, as well as gas and dust – began to form about 13 billion. years ago. Astronomers' observations show that first the largest galaxies were fully formed, and then the turn came to dwarf galaxies, in which the process of star formation continues in our era. The book describes how and why the structure of galaxies has changed over time, what methods we use to investigate the properties of galaxies located in the neighborhood or far from us, and why this particular area of our ideas about the Universe is now rapidly developing and is full of unexpected discoveries every day.
47. Д10-19/66861
Сотникова, Р. Т. Космические лучи и их источники : учебное пособие / Р. Т. Сотникова ; Министерство науки и высшего образования Российской Федерации, Иркутский государственный университет, Физический факультет. – Иркутск : Изд-во ИГУ, 2019. – 139 с. : ил. – Библиогр.: с. 136-139 (60 назв.). – ISBN 978-5-9624-1679-3. – Текст : непосредственный.
Abstract: The textbook is written on the basis of practical research-oriented classes based on modern data on cosmic rays, our Galaxy, quasars, cosmological expansion, solar activity.
48. Р85
Успехи физических наук / Физический институт имени П. Н. Лебедева (Москва), Российская академия наук. – Москва : «Успехи физических наук», ред. журн., 1918 – (Москва). – Перевод заглавия: Progress in Physics (Table of Contents in English). – Выходит ежемесячно. – ISSN 0042-1294. – Текст : непосредственный.
Abstract: A journal that publishes reviews of the current state of the most pressing problems of physics and related sciences. It is intended for researchers, graduate students, senior physics students, teachers.
49. Фесенко, Б. И. Галактики и звёзды / Б. И. Фесенко. – Text : electronic // Вестник Псковского государственного университета. Серия Естественные и физико-математические науки. – 2008. – № 4. – С. 140-141. – ISSN 2227-5193. – URL: https://e.lanbook.com/journal/issue/295150 (дата обращения: 11.04.2022). – Access mode: for authorization. users.
Abstract: The distribution of galaxies in the vicinity of stars brighter than V = 7.25 is being studied. It turned out that in these regions the density of the number of galaxies is somewhat reduced. This result is statistically significant, and it cannot be explained by the direct effect of extended photographic images of stars. Apparently, the presence of dust in the vicinity of some stars, scattering the light of stars and weakening the light of galaxies, affects.
50. Ж2-11/50866
Фридман, А. М. Физика галактических дисков / А. М. Фридман, А. В. Хоперсков. – Москва : Физматлит, 2011 (Чебоксары). – 640 с. : ил. – Библиогр.: с. 588-640 (1332 назв.). – ISBN 978-5-9221-1291-8. – Текст : непосредственный.
Abstract: The physical processes determining the dynamics and spatial structure of astrophysical disks (stellar and gas disks of galaxies) are considered. A consistent study of the dynamics of small disturbances and stability issues for collisionless and gas-dynamic (including accreting) systems is carried out. The physics of numerous instabilities is considered in detail. The main nonlinear results based on numerical (computer) experiments are presented. Some mechanisms of formation of the spiral structure of galaxies are discussed. Approaches to determining the parameters of the dark mass within galaxies and in their immediate vicinity are described. The results of the discovery of new galactic structures in recent years are presented: vortices, slow bars, the soliton structure of spiral arms, and the physics of these phenomena is discussed in detail. For researchers and senior students of physics and mathematics specialties of universities.
51. Д9-09/77126
Химическая и динамическая эволюция галактик : сборник трудов конференции «Химическая и динамическая эволюция галактик», 28-30 сентября 2009 г., Южный федеральный университет, Ростов-на-Дону / Южный федеральный университет (Ростов-на-Дону) ; под редакцией Н. Г. Бочкарева, Ю. А. Щекинова. – Ростов-на-Дону : [б. и.], 2009 (Ростов-на-Дону). – 224 с. : ил. – В надзаг.: Юж. федер. ун-т. – Библиогр. в конце ст. – Авт. указ.: с. 224. – ISBN 978-5-903257-69-0. – Текст : непосредственный.
Abstract: The book deals with a wide range of issues related to the interaction between the stellar and gas components of the Galaxy, its enrichment with heavy elements, mixing of heavy elements in the interstellar medium, the evolution of molecular clouds, etc. The book is of interest both for professional astrophysicists and physicists, undergraduates and graduate students, and for a wide range of readers interested in modern astronomy.
52. Ар18-7829
Хорунжев, Г. А. Поиск и исследование активных ядер галактик и далеких квазаров по данным рентгеновских обзоров неба и наземных телескопов : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Хорунжев Г. А. – Москва, 2018. – 19 с. : ил. – Библиогр.: с. 18-19. – Текст : непосредственный.
53. Д1/34987
Эйгенсон, М. С. Внегалактическая астрономия : введение в изучение галактик / М. С. Эйгенсон ; редактор Т. А. Агекян. – Москва : Гос. изд-во физ.-мат. литературы, 1960. – 414 с. : ил. – Библиогр.: с. 404-414. – Текст : непосредственный.
Abstract: The book is an introduction to the study of extragalactic astronomy as of the late 50s of the twentieth century. One of the introductory chapters is devoted to a brief overview of the history of extragalactic astronomy. Methods and results of measurements of distances of galaxies, their luminosity function, spectral classes and colors are considered.
54. J2/27159
Accretion discs, jets and high energy phenomena in astrophysics = Disques d'accretion, jets et phenomenes de haute energie en astrophysique : NATO ASI, Les houches, Sess. LXXVIII, 29 july – 23 august 2002 / editor V. Beskin. – Berlin [etc.] : Springer, 2003. – XXVII, 625 p. – 625 p. : ill. – Парал. загл. фр. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The accretion process is thought to play a key role in the Universe. This book explains, in a form intelligible to graduate students, its relation to the formation of new stars, to the energy release in compact objects and to the formation of black holes. The monograph describes how accretion processes are related to the presence of jets in stellar objects and active galactic nuclei and to jet formation. The authors treat theoretical work as well as current observational facts. This volume of the highly esteemed Les Houches series is meant as an advanced text that can serve to attract students to exciting new research work in astrophysics.
55. Astrophysical disks : collective and stochastic phenomena / editor A. M. Fridman [et al.]. – Electronic text data. – Dordrecht : Springer, 2006. – 359 p. – ISBN 978-1-4020-4348-2. – URL: http://dx.doi.org/10.1007/1-4020-4348-1 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract:The book deals with collective and stochastic processes in astrophysical discs involving theory, observations, and the results of modelling. Among others, it examines the spiral-vortex structure in galactic and accretion disks, stochastic and ordered structures in the developed turbulence. It also describes sources of turbulence in the accretion disks, internal structure of disk in the vicinity of a black hole, numerical modelling of Be envelopes in binaries, gaseous disks in spiral galaxies with shock waves formation, observation of accretion disks in a binary system and mass distribution of luminous matter in disk galaxies. The editors adaptly brought together collective and stochastic phenomena in the modern field of astrophysical discs, their formation, structure, and evolution involving the methodology to deal with, the results of observation and modelling, thereby advancing the study in this important branch of astrophysics and benefiting Professional Researchers, Lecturers, and Graduate Students.
56. 52(063)/A89-951868
Astrophysics and space science : from X-Ray binaries to quasars: black holes on all mass scales / editor T. J. Maccarone [et al.]. – Electronic text data. – Dordrecht : Springer, 2005. – 288 p. – ISBN 978-1-402-04085-6. – URL: http://dx.doi.org/10.1007/1-4020-4085-7 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: This volume brings together contributions from many of the world's leading authorities on black hole accretion. The papers within represent part of a new movement to make use of the relative advantages of studying stellar mass and supermassive black holes and to bring together the knowledge gained from the two approaches. The topics discussed here run the gamut of the state of the art in black hole observational and theoretical work-variability, spectroscopy, disk-jet connections, and multi-wavelength campaigns on black holes are all covered.
57. Clusters of galaxies : beyond the thermal view / editor J. Kaastra. – Electronic text data // Space Science Reviews. – V 134. – P. 1-6 (2008). – New York, NY : Springer, 2008. – SpringerLink. – ISBN 978-0-387-78875-3. – URL: https://doi.org/10.1007/s11214-008-9326-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: We present the work of an international team at the International Space Science Institute (ISSI) in Bern that worked together to review the current observational and theoretical status of the non-virialised X-ray emission components in clusters of galaxies. The subject is important for the study of large-scale hierarchical structure formation and to shed light on the “missing baryon” problem. The topics of the team work include thermal emission and absorption from the warm-hot intergalactic medium, non-thermal X-ray emission in clusters of galaxies, physical processes and chemical enrichment of this medium and clusters of galaxies, and the relationship between all these processes. One of the main goals of the team is to write and discuss a series of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.
58. R/7069/418
Galactic high-energy astrophysics. High-accuracy timing and positional astronomy : astrophysics school IV, Graz, 19-31 august 1991 / editor J. van Paradijs, editor H. M. Maitzen. – Berlin [etc.] : Springer, 1993. – XI, 293 p. – 293 p. : ill. – (Lecture notes in physics, ISSN 0075-8450 ; 418). – ISBN 3-540-56874-3. – Библиогр. в конце статей. – Текст : непосредственный.
Abstract: This book addresses graduate students in astronomy and astrophysics. The first part is devoted to galactic high-energy astrophysics. It treats particle accelerations (including shocks), the interstellar medium and supernovae remnants, high-energy emissions from normal stars and accretion in close binaries. The second part deals with observationslike pulsar timing, and its measurement with radioastronomical tools, and astrometry, as performed in the HIPPARCOS satellite program.
59. 524.7(063)/G54-291614
Globular clusters – guides to galaxies : proceedings of the Joint ESO-FONDAP Workshop on globular clusters held in Concepcion, Chile, 6-10 march 2006 / editor T. Richtler, S. Larsen. – Berlin ; Heidelberg : Springer, 2009. – 456 p. – (ESO astrophysics symposia, european southern observatory, ISSN 1431-2433). – ISBN 978-3-540-76961-3. – URL: http://dx.doi.org/10.1007/978-3-540-76961-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: The principal question of whether and how globular clusters can contribute to a better understanding of galaxy formation and evolution is perhaps the main driving force behind the overall endeavour of studying globular cluster systems. Naturally, this splits up into many individual problems. The objective of the Joint ESO-FONDAP Workshop on Globular Clusters – Guides to Galaxies was to bring together researchers, both observational and theoretical, to present and discuss the most recent results. Topics covered in these proceedings are: internal dynamics of globular clusters and interaction with host galaxies (tidal tails, evolution of cluster masses), accretion of globular clusters, detailed descriptions of nearby cluster systems, ultracompact dwarfs, formations of massive clusters in mergers and elsewhere, the ACS Virgo survey, galaxy formation and globular clusters, dynamics and kinematics of globular cluster systems and dark matter-related problems. With its wide coverage of the topic, this book constitutes a valuable reference of the scientific knowledge of the field.
60. Keel, William C. The Road to Galaxy Formation / William C. Keel. – Electronic text data. – Berlin ; Heidelberg : Springer : Praxis publ., 2007. – 262 p. – (Springer praxis books). – ISBN 978-3-540-72535-0. – URL: https://doi.org/10.1007/978-3-540-72535-0 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: The formation of galaxies is one of the greatest puzzles in astronomy, the solution is shrouded in the depths of space and time, but has profound implications for the universe we observe today. The book discusses the beginnings of the process from cosmological observations and calculations, considers the broad features of galaxies that we need to explain and what we know of their later history. The author compares the competing theories for galaxy formation and considers the progress expected from new generations of powerful telescopes both on earth and in space.
61. Kim, Dong-Woo. Hot Interstellar Matter in Elliptical Galaxies / Dong-Woo Kim, S. Pellegrini. – Electronic text data. – Dordrecht : Springer, 2012. – 282 p. – (Astrophysics and space science library, ISSN 0067-0057 ; 378). – ISBN 978-1-4614-0580-1. – URL: https://doi.org/10.1007/978-1-4614-0580-1 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Based on a number of new discoveries resulting from 10 years of Chandra and XMM-Newton observations and corresponding theoretical works, this is the first book to address significant progress in the research of the Hot Interstellar Matter in Elliptical Galaxies. A fundamental understanding of the physical properties of the hot ISM in elliptical galaxies is critical, because they are directly related to the formation and evolution of elliptical galaxies via star formation episodes, environmental effects such as stripping, infall, and mergers, and the growth of super-massive black holes. Thanks to the outstanding spatial resolution of Chandra and the large collecting area of XMM-Newton, various fine structures of the hot gas have been imaged in detail and key physical quantities have been accurately measured, allowing theoretical interpretations/predictions to be compared and tested against observational results. This book will bring all readers up-to-date on this essential field of research.
62. 524.7-5/L87-609410
Longair, M. S. Galaxy formation / M. S. Longair. – 2 nd ed. – Electronic text data. – Berlin ; Heidelberg : Springer, 2008. – 737 p. – (Astronomy and astrophysics library, ISSN 0941-7834). – ISBN 978-3-540-73478-9. – URL: http://dx.doi.org/10.1007/978-3-540-73478-9 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: This second edition of Galaxy Formation is an up-to-date text on astrophysical cosmology, expounding the structure of the classical cosmological models from a contemporary viewpoint. This forms the background to a detailed study of the origin of structure and galaxies in the Universe. The derivations of many of the most important results are derived by simple physical arguments which illuminate the results of more advanced treatments. A very wide range of observational data is brought to bear upon these problems, including the most recent results from WMAP, the Hubble Space Telescope, galaxy surveys like the Sloan Digital Sky Survey and the 2dF Galaxy Redshift Survey, studies of Type 1a supernovae, and many other observations.
63. Stahler, S. The Birth of Star Clusters / S. Stahler. – Electronic text data. – Dordrecht : Springer, 2018. – 199 p. – (Astrophysics and space science library, ISSN 0067-0057 ; 424). – ISBN 978-3-319-22801-3. – URL: https://doi.org/10.1007/978-3-319-22801-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: All stars are born in groups. The origin of these groups has long been a key question in astronomy, one that interests researchers in star formation, the interstellar medium, and cosmology. This volume summarizes current progress in the field, and includes contributions from both theorists and observers. Star clusters appear with a wide range of properties, and are born in a variety of physical conditions. Yet the key question remains: How do diffuse clouds of gas condense into the collections of luminous objects we call stars? This book will benefit graduate students, newcomers to the field, and also experienced scientists seeking a convenient reference.
64. Н/14679/1
The formation and evolution of galaxies and their constituents / Академия наук Эстонской ССР. Тартуская астрофизическая обсерватория имени В. Струве. – Tallinn : [б. и.], 19 – . – Текст : непосредственный.
1. – 1988. – 98 p. : il. – Res. rus., angl. – Bibliogr. v konze otd.st.
Abstract: The collection is in English and Russian. Content: 1) M. Gramann. Evolution of perturbations in the cold adiabatic model of the Universe; 2) P. Traat. Types of photometric evolutionary models of galaxies; 3) E. Kazak. About one possible model of the gas corona of the Galaxy; 4) E. Togo. Spatial distribution of clusters of Zwicky galaxies: quantitative tests; 5) P. Tignes. Subsystems in galaxies and their mass-to-luminosity ratios.
65. R/6714/160
Windows on galaxies : proceedings of the sixth workshop of the advanced school of astronomy of the Ettore Majorana centre for scientific culture, Erice, may 21-31, 1989 / Ettore Majorana centre for scientific culture, Advanced school of astronomy ; Comp. G. Fabbiano. – Dordrecht [etc.] : Kluwer, 1990. – XV. – 383 p. : ill. – (Astrophysics and space science library / editor J. E. Blamont ; vol.160). – ISBN 0-7923-0663-5. – Указ.: с.381-383. – Текст : непосредственный.
Abstract: Along with the traditional optical window, many new windows have been opened on galaxies in the last two decades, made possible by new developments in groundbased detectors and by space missions that allow detection of photons that are otherwise absorbed by the Earth's atmosphere. Galaxies can now be observed in the radio, submillimeter, IR, optical, UV, X- and gamma-ray bands, each window allowing us to learn more about galactic components and properties. These developments have also imposed the view that a deeper understanding of even normal galaxies requires a panchromatic approach, making use of all of the data gathered from the different windows to synthesize a comprehensive physical image of these complex astronomical systems. Windows on Galaxies presents a comprehensive view of galaxies through all the available windows, bringing together both theoretical and experimental approaches in the form of a series of reviews reporting the most recent developments complemented by contributed talks and discussions. The sixth workshop of the Advanced School of Astronomy examined galaxies through all available wavelength windows. Over the last twenty years, new wavelength windows have been opened in astronomy which have created many new possibilities for the observation of the properties of galaxies. The outcome of the meeting clearly stated that the approach towards the studying of galaxies should be panchromatic. Each window, from radio to gamma-rays, shows different components, and a synthesis of this knowledge presents astronomers with a comprehensive physical image of these astronomical systems: star formation, evolution of galaxies, molecular contents, gas flows, interstellar matter and properties of galaxies in the several wavelength fields are discussed in this volume.
2. Physics of the interstellar medium
66. Ар17-6986
Андрианов, А. С. Исследование структуры локальной межзвездной плазмы наземно-космическим интерферометром «Радиоастрон» : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Андрианов А. С. – Москва, 2017. – 20 с. : ил. – В надзаг.: Рос. акад. наук. Физ. ин-т им. П. Н. Лебедева. Астрокосм. центр. – Библиогр.: с. 19-20 (12 назв.). – Текст : непосредственный.
67. Ар16-3561
Баяндина, О. С. Свойства молекулярного мазерного излучения в газо-пылевых комплексах Млечного пути : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Баяндина О. С. – Москва, 2016. – 35 с. – Библиогр.: с. 27-35 (75 назв.). – Текст : непосредственный.
68. Ж2-04/35325
Белов, Е. А. Астрофизика. Крабовидная туманность. Черная дыра. g=2,99792458 м/с2 : учебник для астрофизиков / Е. А. Белов. – Москва : Компания Спутник+, 2004. – 184 с. – Библиогр.: с. 180. – ISBN 5-93406-819-9. – Текст : непосредственный.
69. Д7-90/80560
Бочкарев, Н. Г. Местная межзвездная среда / Н. Г. Бочкарев. – Москва : Наука, 1990. – 189 c. : ил. – ISBN 5-02-014351-0. – Библиогр.: с. 156-177. – Указ.: с. 179-189. – Текст : непосредственный.
Abstract: Various observational data on the local interstellar medium – a region with a radius of about 200 km in the vicinity of the Sun - were collected and analyzed: radio, infrared, optical, X-ray and gamma–ray observations of the interstellar medium, as well as information about the Scorpio-Centauri stellar association. The local interstellar medium is a section of a vast region of star formation associated with the Gould Belt. It contains a giant cavern of hot rarefied gas, bordered by cold gas-dust fibers. This cavern and shell are formed by the action of the stellar wind and supernova flares in the Scorpio–Centauri association. Inside it there is an unusually large supernova remnant – the North Polar Hole. The study of the local interstellar medium sheds light on many nodal problems of the physics of the interstellar medium and the evolution of the Galaxy. Knowledge of the parameters of the local interstellar medium is necessary to reduce observations of both extragalactic objects and radiation sources located in the Galaxy, in order to understand the environment in which the Solar System is located. Designed for specialists in the field of astrophysics, stellar astronomy and physics, as well as graduate students of relevant specialties.
70. Д9-10/67022
Бочкарев, Н. Г. Основы физики межзвездной среды : учебное пособие / Н. Г. Бочкарев. – 2-е изд. – Москва : URSS, 2010. – 351 с. : ил. – ISBN 978-5-397-01034-4. – Текст : непосредственный.
Abstract: The textbook is written in accordance with the program of the course "Theoretical Astrophysics" and contains information on the theory of observation methods and physical processes in the areas of neutral hydrogen in the interstellar medium, on molecules in interstellar space, cosmic masers, the structure of the interstellar medium, interstellar dust. Along with the classical sections of the physics of the interstellar medium, the results obtained in recent decades and not included in the previously existing textbooks are considered. The manual is intended for students of physics faculties of universities studying in the specialty "astronomy", for teachers, as well as researchers of physical and astronomical specialties.
71. Д10-18/55273
Бычков, К. В. Непрерывный спектр излучения звёздных атмосфер и межзвёздной среды : учебное пособие для студентов специальности «Астрономия» / К. В. Бычков, О. М. Белова. – Москва : ГАИШ МГУ, 2018. – 99 с. : ил. – ISBN 978-5-4465-1835-7. – Текст : непосредственный.
Abstract: Using the example of free-free and bound-free transitions of hydrogen plasma, the physical foundations of the interaction of the radiation field with matter are described. The basic concepts of the theory of radiation are given, the transfer equations and the condition of radiant equilibrium are derived taking into account the forced radiation. An idea of elementary processes, the principle of detailed balance, full and partial thermodynamic equilibrium is given. The conditions under which the transfer equation admits a form with "enlightenment", when forced radiation can be considered as attenuation of absorption, are clarified. Kirchhoff's law is discussed for cases of complete and partial thermodynamic equilibrium. The problem of the transfer of radio emission in the ionized gas of the interstellar medium is solved. A comparative analysis of known methods for solving the transport equation in a "gray" atmosphere, that is, in the atmosphere of a star with a frequency-independent absorption coefficient, is performed. The question of complete and partial thermodynamic equilibrium in the interstellar medium and stellar atmospheres is considered.
72. М/14605/ИТФ-91-66Р
Головатый, В. В. Современная фотоионизационная модель свечения планетарной туманности : краткое описание / В. В. Головатый, Ю. Ф. Мальков. – Киев, 1991. – 41 с. – (Препринт / Институт теоретической физики (Киев) ; ИТФ-91-66Р). – Текст : непосредственный.
Abstract: An algorithm for constructing and self-matching a modern photoionization model of the glow of a planetary nebula is described. All processes that play an important role in establishing the ionization and thermal equilibrium of the nebular gas are taken into account. Diffuse ionizing radiation is fully taken into account. The model is constructed for the radial distribution of the gas density in the nebula, consistent with its map in some Balmer line or radio continuum.
73. М/42146/111
Госачинский, И. В. Статистические характеристики облаков межзвездного нейтрального водорода / И. В. Госачинский, В. В. Морозов. – Санкт-Петербург : [б. и.], 1995. – 16 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 111). – Текст : непосредственный.
Abstract: This paper presents the results of calculating the spectra of linear sizes, concentrations and masses of neutral hydrogen for about 5000 HI clouds detected in the radiation line at a wave of 21 cm on the RATAN-600 radio telescope in the region of 180o <1 <260o and – 15o
74. Ар11-8614
Егоров, О. В. Исследование газовой и пылевой составляющих межзвездной среды в галактиках с бурным звездообразованием IC 10 и VII ZW 403 : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Егоров О. В. – Москва, 2011. – 16 с. – В надзаг.: МГУ им. М. В. Ломоносова, Гос. астроном. ин-т им. П. К. Штернберга. – Библиогр.: с. 14-16 (19 назв.). – Текст : непосредственный.
75. М/16400/9 за 2017 г.
Елизарова, Т. Г. О возможностях квазигазодинамической модели для численного анализа сверхзвукового турбулентного течения межзвездного газа / Т. Г. Елизарова, И. А. Широков, М. В. Попов. – Москва : ИПМ им. М. В. Келдыша РАН, 2017. – 21 с. : ил. – (Препринт / Институт прикладной математики им. М. В. Келдыша (Москва) ; 9 за 2017 г.). – Библиогр.: с. 20-21 (22 назв.). – ISSN 20712898. – Текст : непосредственный
Abstract: The results of numerical simulation of interstellar gas clouds, performed for the first time in the framework of a quasi-gas dynamic (CGD) algorithm, are presented. The decay of a Taylor-Green vortex and a quasi-stationary flow with an initial condition in the form of a random solenoid velocity field with an energy source are considered. Typical parameters of interstellar gas clouds in which stars can form were used. The results obtained show the capabilities of the CGD algorithm for modeling sparse large-scale turbulent clouds, including a supersonic flow zone.
76. Ар09-4461
Зиракашвили, В. И. Гидродинамические и плазменные эффекты космических лучей в Галактике : специальность 01.04.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Зиракашвили В. И. – Москва, 2009. – 38 с. : ил. – Библиогр.: с. 34-38 (77 назв.). – Текст : непосредственный.
77. Д1/10920
Каплан, С. А. Межзвездная газодинамика / С. А. Каплан. – Москва : Физматгиз, 1958. – 194 с. : ил. – Библиогр.: с. 192-194 (97 назв.). – Текст : непосредственный.
Abstract: A cursory glance at the astrophysical literature of recent years shows how much the specific weight of studies of gas movements in interstellar space and in stellar atmospheres (cosmic gas dynamics and cosmic electrodynamics) has increased. The development of these fields of astrophysics is also facilitated by the great attention currently being paid to cosmogony, a science that, in essence, is based on the study of the movements of gas and dust in cosmic conditions. The problems of cosmic gas dynamics and magnetic hydrodynamics have been discussed to one degree or another at almost all astrophysical conferences and meetings in recent years. However, despite the great importance of space gas dynamics and the abundance of journal literature on these issues, there are still no more or less systematic studies of gas dynamic gas movements in space conditions.
78. Ар16-5566
Клименко, В. В. Исследование физических условий в облаках молекулярного водорода с большими красными смещениями : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Клименко В. В. – Санкт-Петербург, 2016. – 18 с. : ил. – Библиогр.: с. 16-18 (38 назв.). – Текст : непосредственный.
79. М/16400/61 за 2014 г.
Колесниченко, А. В. Термодинамическая модель сжимаемой магнитогидродинамической турбулентности космической плазмы / А. В. Колесниченко. – Москва : ИПМ им. М. В. Келдыша РАН, 2014. – 48 с. – (Препринт / Институт прикладной математики им. М. В. Келдыша (Москва) ; № 61 за 2014). – Библиогр.: с. 47-48 (25 назв.). – Текст : непосредственный.
Abstract: In the approximation of single-fluid magnetic hydrodynamics, a closed system of MHD equations of the mean motion scale is obtained, designed to simulate compressible turbulent flows of electrically conductive media in the presence of a magnetic field. In order to visually interpret the individual components of the energy balance of the plasma and the field, various energy equations are obtained that allow tracing possible energy transitions from one form to another, in particular, to understand the mechanisms of pumping the gravitational and kinetic energy of the average motion into magnetic energy. Special attention is paid to the method of obtaining, within the framework of extended irreversible thermodynamics, closing relations for the complete (taking into account the magnetic field) kinetic tensor of turbulent stresses and the so-called magnetic Reynolds tensor, which also allows analyzing the restrictions imposed by the entropy increase condition on the turbulent transport coefficients. A method for modeling the coefficients of turbulent transport, in particular, the coefficient of kinematic turbulent viscosity, is proposed, taking into account the influence of the magnetic field and the reverse effect of heat transfer on the development of turbulence in an electrically conductive medium.
80. Ар17-3697
Кочина, О. В. Диагностика физических условий в областях звездообразования при помощи химического моделирования : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Кочина О. В. – Москва, 2017. – 17 с. – Библиогр.: с. 14-17. – Текст : непосредственный.
81. Ар16-6353
Ладейщиков, Д. А. Исследование пространственно-кинематической структуры гигантских молекулярных облаков : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Ладейщиков Д. А. – Екатеринбург, 2016. – 19 с. – В надзаг.: Урал. федер. ун-т им. первого Президента России Б. Н. Ельцина. – Библиогр.: с. 16-18. – Текст : непосредственный.
82. Д7-90/82986
Математические модели ближнего космоса : II Всесоюзное совещание, посвященное памяти В. П. Шабанского, Москва, 1990 г. : тезисы докладов / редакционная коллегия: А. П. Кропоткин (ответственный редактор) [и др.]. – Москва, 1990. – 77 с. : ил. – В надзаг.: МГУ им. М. В. Ломоносова, НИИ ядерной физики. – Библиогр. в конце докл. – Текст : непосредственный.
Abstract: The collection contains abstracts of reports presented at the II All-Union Meeting on the Theory and Mathematical Modeling of phenomena in near-Earth and near-solar space. The works are grouped into the following main areas: 1) space electrodynamics; magnetic hydrodynamics; 2) magnetosphere radiation belts; magnetospheric-ionospheric interaction; 3) ionosphere and thermosphere; 4) cosmic rays; 5) Sun, solar wind; 6) active experiments.
83. М/11751/39
Межзвездная среда : сборник статей / под редакцией Г. М. Рудницкого. – Москва : [б. и.], 1990. – 158 с. : ил. – (Астрономия / ВИНИТИ ; т.39). – На обл. только загл. сер. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: 1) The review contains the results of the study of the interstellar medium using the COPERNICUS and IUE satellite, the results of studies on the energy and the full composition of the rarefied phases of the interstellar medium, the mechanisms of formation of multicharged ions in the disk and corona of the Galaxy; the properties of interstellar gas regulated by supernova outbreaks are given. 2) Review of observational data in the theoretical view of the interstellar magnetic field; the role of the magnetic field in the process of star formation, in the physics of instabilities, ambipolar diffusion is discussed.
84. Ар20-2297
Мингалев, О. В. Описание крупномасштабных процессов в бесстолкновительной космической плазме и численное моделирование тонких токовых слоев : специальность 01.03.03 – Физика Cолнца : автореферат диссертации на соискание ученой степени доктора физико-математических наук / Мингалев Олег Викторович. – Апатиты, 2020. – 32 с. – Библиогр.: с. 30-32 (21 назв.). – Текст : непосредственный.
85. М/9354/10(2015)
Миронова, Е. Н. Пыль в солнечной системе / Е. Н. Миронова. – Москва : ФИАН им. П. Н. Лебедева, 2015. – 12 с. – (Препринт / Физический ин-т им. П. Н. Лебедева (Москва) ; 10 (2015)). – Библиогр.: с. 12 (33 назв.). – Текст : непосредственный.
Abstract: A brief overview of modern ideas about the interplanetary dust cloud.
86. Ар19-7480
Моисеенко, Д. А. Энерго-масс анализаторы для исследования солнечной плазмы и межпланетной пыли. Моделирование. Принципы создания : специальность 01.03.03 – Физика Cолнца : автореферат диссертации на соискание ученой степени кандидата физико-математических наук / Моисеенко Д. А. ; Московский государственный университет имени М. В. Ломоносова. – Москва, 2019. – 24 с. : ил. – Библиогр.: с. 23-24 (19 назв.). – Текст : непосредственный.
Abstract: The results of the author's work on the creation of ion energy-mass analyzers for the study of the Sun, the interplanetary medium and near–planetary space are presented - from the formulation of the problem of a space experiment, the creation of numerical models and laboratory models, participation in the development and manufacture of devices, their tuning and testing, and to the development of experimental methods using manufactured samples of devices.
87. Ар21-4931
Молярова, Т. С. Химическая структура протопланетных дисков со стационарной и вспышечной аккрецией : специальность 01.03.02 – Астрофизика и звёздная астрономия : автореферат диссертации на соискание ученой степени кандидата физико-математических наук / Молярова Тамара Сергеевна ; Институт астрономии Российской академии наук. – Москва, 2021. – 20 с. : ill. – Библиогр.: с. 16-20. – Текст : непосредственный.
88. Ар15-2391
Мурга, М. С. Эволюция пыли во внегалактических областях ионизованного водорода : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Мурга М. С. – Санкт-Петербург, 2015. – 16 с. – Библиогр.: с. 14-16. – Текст : непосредственный.
89. Ар16-6355
Павлюченков, Я. Н. Излучение молекул и пыли в дозвездных и протозвездных объектах : специальность 01.03.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Павлюченков Я. Н. – Москва, 2016. – 22 с. – В надзаг.: Рос. АН, Ин-т астрономии. – Библиогр.: с. 18-22. – Текст : непосредственный.
90. Ар18-4018
Петров, А. Е. Динамические магнитные структуры в сильнонеравновесной релятивистской плазме пульсарных туманностей : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Петров А. Е. – Санкт-Петербург, 2018. – 18 с. : ил. – Библиогр.: с. 16-18. – Текст : непосредственный.
91. Д1/11652
Пикельнер, С. Б. Физика межзвездной среды / С. Б. Пикельнер ; Академия наук СССР. – Москва : Изд-во Академии наук СССР, 1959. – 215, [1] с. : ил. – (Научно-популярная серия). – Текст : непосредственный.
Abstract: The book is written on an urgent topic of great importance, first of all, in cosmogonic terms. The author presents in a simple and accessible form quite complex and diverse processes occurring in the interstellar medium, and their connection with the processes occurring in the stars. To facilitate the understanding of these issues, the Introduction briefly introduces the reader to the stars and our Galaxy. The author shows that the study of the interstellar medium is closely connected with the most important problem of astronomy – the problem of the origin and evolution of stars. A summary of the current state of this problem is given very vividly and is read with great interest.
92. Поройков, С. Ю. Вклад давления межгалактической среды на короны галактик и их взаимное отталкивание / С. Ю. Поройков. – Text : electronic // Журнал естественнонаучных исследований. – 2019. – № 2. – С. 8-19. – URL: https://znanium.com/catalog/product/1066490 (дата обращения: 27.04.2022). – Access mode: for authorization. users.
Abstract: It is shown that the pressure of cosmic rays of the observed energy density on the corona of galaxies compensates for the gravitational attraction of typical galaxies, taking into account the hidden mass of their corona. The energy release corresponding to the cosmic ray flux can be provided by type II supernovae during the gravitational collapse of their nuclei into neutron stars. The contribution of the pressure of microwave background radiation on the corona of galaxies during its scattering by hot electrons of coronal gas is estimated. It is shown that these factors will ensure the expansion of a homogeneous closed Riemannian Universe, beyond the cosmological horizon of which there is matter.
93. Ар15-1022
Прудских, В. В. Коллективные явления в пылевой астрофизической плазме : специальность 01.04.03 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Прудских В. В. – Ростов-на-Дону, 2014. – 32 с. : ил. – Библиогр.: с. 28-32. – Текст : непосредственный.
94. Н/8229/ФЭИ-3035
Рыков, В. А. Аналогия в форме структур пылевых частиц в трековой плазме и объектов во Вселенной / В. А. Рыков, К. В. Рыков, И. А. Денежкин. – Обнинск : [б. и.], 2004. – 23 с. : ил. – (Препринт / Физико-энергетический ин-т им. А. И. Лейпунского (Обнинск) ; ФЭИ-3035). – Библиогр.: с. 22-23(45 назв.). – Текст : непосредственный.
Abstract: This paper presents the results of an experimental study of the behavior of dust particles in a track plasma created by a beam of accelerated protons and in a nuclear-excited plasma. The obtained collective effects in dust structures are compared with the results of observations of objects in the Universe. There are similar external features in the structures and their behavior.
95. Д9-08/77124
Субпарсековые структуры в межзвездной среде : сборник трудов семинара рабочей группы по межзвездной среде, прошедшего 4-5 июля 2007 года ГАИШ, Москва / Государственный астрономический институт имени П. К. Штернберга ; под редакцией Н. Г. Бочкарева, Ю. А. Щекинова. – Москва : Изд-во РСЭИ, 2008 (Ростов-на-Дону). – 184 с. : ил. – Библиогр. в конце ст. – ISBN 978-5-903257-70-6. – В надзаг.: Гос. астроном. ин-т им. П. К. Штернберга. – Текст : непосредственный.
Abstract: The purpose of the seminar was to exchange opinions of specialists on the formulated problems. The collection deals with a wide range of issues related to the origin of the structure in the interstellar medium and the physics of star formation, especially in a substance with a primary chemical composition; the impact of shock waves on the interstellar medium, the destruction of interstellar clouds by shock waves, mixing of chemical inhomogeneities, dynamics and structure of nuclei of molecular clouds, etc. The book is of interest both for professional astrophysicists and physicists, and for a wide range of readers interested in modern astronomy.
96. М/20361/5(1990)
Сурдин, В. Г. Гигантские молекулярные облака / В. Г. Сурдин. – Москва : Знание, 1990. – 64 c. – (Новое в жизни, науке, технике... Серия «Космонавтика, астрономия» ; 5 (1990)). – ISBN 5-07-000516-2. – Текст : непосредственный.
Abstract: The brochure tells about the history of the discovery and the observed characteristics of giant molecular clouds, about the possible mechanisms of their formation and destruction, about their connection with the process of star formation and other evolutionary processes in the Galaxy. The brochure is intended for a wide range of readers.
97. Ар20-3472
Топчиева, А. П. Морфология и эволюция инфракрасных кольцевых туманностей вокруг областей ионизованного водорода : специальность 01.03.02 – Астрофизика и звездная астрономия : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Топчиева Анастасия Павловна. – Москва, 2020. – 27 с. – Библиогр.: с. 20-27. – Текст : непосредственный.
98. Ар08-5452
Чернышов, А. А. Исследование сжижаемой магнитогидродинамической турбулентности в космической плазме методом крупных вихрей : специальность 01.04.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Чернышов А. А. – Москва, 2008. – 20 с. – Библиогр.: с. 19-20. – Текст : непосредственный.
99. Ар13-16186
Шевелев, М. М. Неустойчивость Кельвина-Гельмгольца для потока плазмы, ограниченного в пространстве : специальность 01.04.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Шевелев М. М. – Москва, 2013. – 26 с. : ил. -Библиогр.: с. 25-26. – Текст : непосредственный.
100. Astrophysics. – Electronic text data. – Heidelberg : Springer-RL-Verl., 1965 – . – Выходит ежеквартально. – ISSN 0571-7256. – Загл. с титул. экрана. – URL: http://www.springerlink.com/content/0571-7256 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Presents recent theoretical and experimental advances in astrophysics. Covers planetary atmospheres, interstellar matter, solar physics, and space astrophysics.
101. 523-726/C21-245003
Cargill, P. Turbulence in space plasmas / P. Cargill, L. Vlahos. – Electronic text data. – Berlin ; Heidelberg : Springer, 2009. – 325 p. – (Lecture notes in physics, ISSN 0075-8450; 778). – ISBN 978-3-642-00210-6. – URL: http://dx.doi.org/10.1007/978-3-642-00210-6 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Over the years, many leading European graduate schools in the field of astrophysical and space plasmas have operated within the framework of the research network, «Theory, Observations, and Simulations in Turbulence in Space Plasmas». This text is a set of lectures and tutorial reviews culled from the relevant work of all those schools. It emphasizes applications on solar coronae, solar flares, and the solar wind. In bridging the gap between standard textbook material and state-of-the-art research, this text offers a broad flavor to postgraduate and postdoctoral students just coming to the field. And because of its unique mix, it will also be useful to lecturers looking for advanced teaching material for their seminars and courses.
102. Dense molecular gas around protostars and in galactic nuclei : european workshop on astronomical molecules 2004 / editor W. Baan [et al.]. – Electronic text data. – Dordrecht : Springer, 2005. – 330 p. – ISBN 978-1-402-03831-0. – URL: http://dx.doi.org/10.1007/1-4020-3831-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Covers maser and dense gas diagnostics and related phenomena, evolution of circumstellar regions around protostars, evolution of circumnuclear regions of active galaxies, diagnostics of the circumnuclear gas in stars and galactic nuclei. Summarizes our present knowledge in these topics, highlights major problems to be addressed, and finally proposes future work.
103. From the outer heliosphere to the local bubble : comparisons of new observations with theory / editor J. L. Linsky [et al.]. – Electronic text data. – Berlin ; Heidelberg : Springer, 2009. – 478 p. – (Space sciences series of issi, ISSN 1385-7525 ; 31). – ISBN 978-1-441-90247-4. – URL: http://dx.doi.org/10.1007/978-1-4419-0247-4 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: The present volume provides a state-of-the-art synopsis of our current understanding of the dynamic heliosphere, the interstellar clouds surrounding it, the wider neighborhood of the local bubble, and their complex interactions. It is written by many of the researchers who have made key discoveries, observations, and modeling efforts that have led to dramatic progress in the field over the past 25 years. Thus the book is an essential research tool for space scientists and astronomers alike, including graduate students for whom it presents a single-point entrance into this complex yet fascinating field.
104. G2/16039
Gierens, K. M. Ein neues Strahlungstransportmodell f:ur interstellare Molekülwolken : dissertation / K. M. Gierens. – Köln, 1990. – 114 S. : Ill. – Библиогр.: с. 111-114. – Текст : непосредственный.
105. Kappa Distributions. From Observational Evidences via Controversial Predictions to a Consistent Theory of Nonequilibrium Plasmas / editor M. Lazar [et al.]. – Electronic text data. – Dordrecht : Springer, 2021. – 330 p. – (Astrophysics and space science library, ISSN 0067-0057 ; 464). – ISBN 978-3-030-82623-9. – URL: https://doi.org/10.1007/978-3-030-82623-9 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: This book presents recent results on the modelling of space plasmas with Kappa distributions and their interpretation. Hot and dilute space plasmas most often do not reach thermal equilibrium, their dynamics being essentially conditioned by the kinetic effects of plasma particles, i.e., electrons, protons, and heavier ions. Deviations from thermal equilibrium shown by these plasma particles are often described by Kappa distributions. Although well-known, these distributions are still controversial in achieving a statistical characterization and a physical interpretation of non-equilibrium plasmas. The results of the Kappa modelling presented here mark a significant progress with respect to all these aspects and open perspectives to understanding the high-resolution data collected by the new generation of telescopes and spacecraft missions. The book is directed to the large community of plasma astrophysics, including graduate students and specialists from associated disciplines, given the palette of the proposed topics reaching from applications to the solar atmosphere and the solar wind, via linear and quasilinear modelling of multi-species plasmas and waves within, to the fundamental physics of nonequilibrium plasmas.
106. Klein, U. Galactic and Intergalactic Magnetic Fields / U. Klein, A. Fletcher. – Electronic text data. – Cham : Springer, 2015. – 236 p. – (Springer Praxis Books). – ISBN 978-3-319-08942-3. – URL: https://link.springer.com/book/10.1007/978-3-319-08942-3 (дата обращения 11.04.2022). – Access mode: for authorization. users.
Abstract: Conveys the fundamentals of magnetic fields and relativistic plasma in diffuse cosmic media. Addresses theoretical concepts wherever necessary. Discusses the role of magnetic fields in the evolution of the interstellar medium, galaxies and galaxy clusters.
107. J2/26512
Kristen, H. Dynamics of the interstellar matter in galaxies : Isolated barred spiral galaxies. Cloud formation processes : dissertation / H. Kristen. – Stockholm, 1998. – Pag. var. : ill. – Библиогр. в конце разделов. – ISBN 91-7153-761-9. – Текст : непосредственный.
Abstract: The dynamical components of six isolated barred spiral (SB) galaxies are investigated. No evidence is found supporting the hypothesis of a low amount of dark matter being characteristic of SB galaxies. The presence of companion galaxies is found to correlate with an increased statistical spread in the neutral hydrogen (HI) extent. It is concluded that the selection of galaxies with large HI extent may introduce a bias towards tidally interacting systems.
108. Lequeux, J. The interstellar medium / J. Lequeux. – Electronic text data. – Berlin ; Heidelberg : Springer, 2005. – 440 p. – (Astronomy and astrophysics library, ISSN 0941-7834). – ISBN 978-3-540-26693-8. – URL: http://dx.doi.org/10.1007/b137959 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Describing interstellar matter in our galaxy in all of its various forms, this book also considers the physical and chemical processes that are occurring within this matter. The first seven chapters present the various components making up the interstellar matter and detail the ways that we are able to study them. The following seven chapters are devoted to the physical, chemical and dynamical processes that control the behaviour of interstellar matter. These include the instabilities and cloud collapse processes that lead to the formation of stars. The last chapter summarizes the transformations that can occur between the different phases of the interstellar medium. Emphasizing methods over results, «The Interstellar Medium» is written for graduate students, for young astronomers, and also for any researchers who have developed an interest in the interstellar medium.
109. V1206/2012, N 195
Nonequilibrium dynamics in astrophysics and materials science : proccedings of the international workshop, Yukawa inst. for theoretical physics, Kyoto university, Oct. 31-Nov. 3, 2011 / editor H. Hayakawa. – Kyoto : Phys. soc. of Japan, 2012. – VII, 200 p. : ill. – (Progress of theoretical physics. Supplement, ISSN 0375-9687 ; 2012, N 195). – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: This workshop is an interdisciplinary one among astrophysics, nuclear physics and condensed matter physics. The aim of the workshop is to encourage the communication between different fields and to find universal structure in nonequilibrium dynamics in various fields. Indeed, there are plenty of examples of nonequilibrium dynamics in astronomical environment and collision of nuclear matter. Thus, it is a good occasion to think of application of new methods in nonequilibrium physics to describe phenomena observed in such fields. In this workshop, we will focus the three fields, jet processes in astronomy, heavy nuclear collisions and granular materials, the formation of planetary rings based on granular kinetic theory, physics of fluid turbulence and its application to various fields. The organizers will welcome young and flexible researchers who are interested in broad fields of science.
110. W12317
Physics of Plasmas. – [S. l.] : AIP Publishing. – Выходит ежемесячно. – До 1994г. см.: Physics of Fluids B : Plasma Physics. – ISSN 0899-8221. – ISSN 1070-664X. – Текст : непосредственный.
Abstract: Articles, reviews and reports on the results of theoretical and experimental studies in the field of plasma physics, including magnetic hydrodynamics, kinetic theory and statistical mechanics of fully or partially ionized gases: general properties and elementary processes in plasma; equilibrium, linear waves and instabilities; nonlinear behavior (including turbulence and stochastic phenomena, solitons and shock waves); physics of lasers and particle beams, acceleration and transfer of charged particles, accelerators; generation, transfer and propagation of radiation, interaction of radiation with plasma; low-temperature plasma and its sources; gas-discharge plasma; plasma chemistry; geophysical, space and astrophysical plasma; magnetic and inertial plasma confinement, tokamaks; physics of high-energy dense plasma or matter under extreme conditions; dust plasma; mathematical descriptions, modeling and numerical methods in plasma physics.
111. Piel, A. Plasma physics : an introduction to laboratory, space, and fusion plasmas / A. Piel. – Electronic text data. – Berlin ; Heidelberg : Springer, 2010. – 398 p. – ISBN 978-3-642-10491-6. – URL: http://dx.doi.org/10.1007/978-3-642-10491-6 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Different from most introductory texts, modern fields of plasma physics, such as low-temperature plasmas, plasma discharges and plasma diagnostics are covered. Emphasis on experimental point of view and laboratory applications. Gives introduction to forefront research on complex plasmas, like non-neutral or dusty plasmas.
112. Planetary nebulae beyond the milky way : proceedings of the ESO workshop held at Garching, Germany, 19-21 May, 2004 / editor L. Stanghellini [et al.]. – Electronic text data. – Berlin ; Heidelberg : Springer, 2006. – 372 p. – (ESO astrophysics symposia european southern observatory, ISSN 1611-6143). – ISBN 978-3-540-34270-0. – URL: http://dx.doi.org/10.1007/11604792 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: In the last decade extra-galactic planetary nebulae (PNe) have gained increasing importance. Improved observational capabilities have allowed fainter and fainter PNe to be studied in galaxies well beyond the Milky Way. Planetary nebulae can be detected to at least 30Mpc. They are found in galaxies of all types and also between the galaxies in nearby galaxy clusters. They are valuable as probes, both for providing the velocity of their host stars and also the evolutionary status and relation to the stellar population from which they formed. This book contains the proceedings of a workshop held at ESO headquarters in Garching in 2004, the first meeting devoted entirely to Extra-galactic Planetary Nebulae. A wide range of topics is covered, from stellar and nebular astrophysics to galactic dynamics and galaxy clusters, making this volume a unique and timely reference of broad astrophysical interest.
113. Recent advances in spectroscopy : theoretical, astrophysical and experimental perspectives / editor R. K. Chaudhuri [et al.]. – Electronic text data. – Berlin ; Heidelberg : Springer, 2010. – (Astrophysics and space science proceedings, ISSN 1570-6591). – ISBN 978-3-642-10322-3. – URL: http://dx.doi.org/10.1007/978-3-642-10322-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: In recent years there have been great advances in the fields of laboratory and astronomical spectroscopy. These have been equally matched by large-scale computations using state-of-the-art theoretical methods. The accurate atomic opacities that are available today play a great role in the field of biomedical research using nanotechnology. The proceedings of the «International Conference on Recent Advances in Spectroscopy: Theoretical, Experimental and Astrophysical Perspectives» contain both invited and contributory papers, which give the most recent results by the peers in the areas of theoretical and experimental atomic physics as well as observational astrophysics.
114. 523-726/S71-483304
Somov, B. V. Plasma astrophysics / B. V. Somov. – Electronic text data. – New York, NY : Springer Science + Business Media LLC, 2007. – 842 p. – (Astrophysics and space science library, ISSN 0067-0057 ; 341). – ISBN 978-0-387-68894-7. – URL: http://dx.doi.org/10.1007/978-0-387-68894-7 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: This well-illustrated monograph is devoted to classic fundamentals, current practice, and perspectives of modern plasma astrophysics. The first part is unique in covering all the basic principles and practical tools required for understanding and working in plasma astrophysics. The second part presents the physics of magnetic reconnection and flares of electromagnetic origin in space plasmas within the solar system; single and double stars, relativistic objects, accretion disks, and their coronae are also covered. This book is designed mainly for professional researchers in astrophysics. However, it will also be interesting and useful to graduate students in space sciences, geophysics, as well as advanced students in applied physics and mathematics seeking a unified view of plasma physics and fluid mechanics.
115. 523-726/S71-840086
Somov, B. V. Plasma astrophysics, part 1 : fundamentals and practice / B. V. Somov. – Electronic text data. – New York, NY : Springer Science + Business Media LLC, 2006. – 444 p. – (Astrophysics and space science library ; 340). – ISBN 978-0-387-48427-3. – URL: http://dx.doi.org/10.1007/978-0-387-48427-3 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: In the book, brief historical remarks demonstrate that the outstanding discoveries in cosmic physics were by no means governed by chance. Distinguishing feature of the proposed book is the consecutive consideration of physical principles, starting from the most general ones (the first principles), and of the simplifying assumptions which give us more and more simpler descriptions of plasma under cosmic conditions.
116. R/7069/350
Structure and dynamics of the interstellar medium : proceedings of IAU Colloquium No. 120 Held on the Occasion of Guido’s Jubilee in Granada, Spain, April 17-21, 1989 / editor G. Tenorio-Tagle. – Berlin : Springer, 1989. – XXI. – 537 p. : ill. – (Lecture notes in physics, ISSN 0075-8450; N350). – Библиогр. в конце ст. – ISBN 3-540-51956-4. – Текст : непосредственный.
Abstract: Here for the first time is a book that treats practically all aspects of modern research in interstellar matter astrophysics. 20 review articles and 40 carefully selected and refereed papers give a thorough overview of the field and convey the flavor of enthusiastic colloquium discussions to the reader. The book includes sections on: – Molecular clouds, star formation and HII regions – Mechanical energy sources – Discs, outflows, jets and HH objects – The Orion Nebula – The extragalactic interstellar medium – Interstellar matter at high galactic latitudes – The structure of the interstellar medium.
117. R/6714/161
<The>interstellar medium in galaxies : invited talks presented at the second Wyoming conference, held at Grand Teton National Park, Wyoming, USA, July 3-7, 1989 / editor Thronson (jr) H. A. – [S. l. : s. n.], 1990. – VIII. – 556 p. : ill. – (Astrophysics and space science library / editor : J. E. Blamont ; vol. 161). – ISBN 0-7923-0759-3. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The Interstellar Medium in Galaxies – An Overview G. R. Knapp. The Cool Phase of the Interstellar Medium: Atomic Gas E. Brinks. Molecular Clouds in Spiral Galaxies J. Young. Interstellar Dust in Galaxies M. Rowan-Robinson. The Effects of Environment on the Cool Phase of the Interstellar Medium in Galaxies J. D. P. Kenney. The Diffuse Interstellar Medium D. P. Cox. Cooling Flows and X-Ray Emission in Early-Type Galaxies C. L. Sarazin. The Interstellar Medium in Active Galaxies J. H. Krolik. Abundances in Extragalactic HII Regions H. L. Dinerstein. Thermal Phases of the Interstellar Medium in Galaxies M. C. Begelman. Large Scale Interstellar Gasdynamics in Disk Galaxies S. A. Balbus. Gas During Mergers/Collisions M. Noguchi. Magnetic Fields in Galaxies R. Wielebinski. The Early ISM and Galaxy Formation S. D. M. White. Gaseous Halos and Disks of Galaxies at Large Redshift A. M. Wolfe. Large Scale Star Formation and the Interstellar Medium R. C. Kennicutt. The Star-Gas Cycle in Galaxies M. A. Dopita. Measuring Atomic Hydrogen Masses Using the 21-CM Line J. M. Dickey. Mass Determinations from Far-Infrared Observations B. T. Draine. Mass Determinations from CO Observations P. Maloney. The M51 System: Review of the Interstellar Medium R. J. Rand, R. P. J. Tilanus. Interstellar Medium in External Galaxies J. P. Ostriker.
118. R/7069/331
The physics and chemistry of interstellar molecular clouds: mm and Sub-mm observations in astrophysics : proceedings of a Symposium Held at Zermatt, Switzerland, 22-25 September 1988 to Commemorate the 600th Anniversary of the University of Cologne and the 20th Anniversary of the Gornergrat Observatory / editor G. Winnewisser, J. T. Armstrong. – Berlin: Springer, 1989. – XVIII. – 463 p. : ill. – (Lecture notes in physics, ISSN 0075-8450 ; N 331). – Библиогр. в конце ст. – Указ.: с.445-460. – ISBN 3-540-51297-7. – Текст : непосредственный.
Abstract: The purpose of this book is to contribute to improved understanding of interstellar physics and chemistry. The most recent results in the field of millimeter, submillimeter and infrared astronomy are presented, with an emphasis on galactic and extragalactic interstellar molecular spectroscopy. The topics are treated both in the form of review articles and short communications. The presentation guides the newcomer to the most advanced topics both in the astrophysical and in the technical development, as well as covering the history of the subject. As a comprehensive overview the book will be useful for researchers and postgraduates.
119. 523-726(063)/T95-185948
Turbulence, dynamos, accretion disks, pulsars and collective plasma processes : first Kodai-Trieste workshop on plasma astrophysics held at the Kodaikanal observatory, Kodaikanal, India, August 27 – September 7, 2007 / editor S. S. Hasan [et al.]. – Electronic text data. – Dordrecht : Springer, 2008. – 342 p. – (Astrophysics and space science proceedings, ISSN 1570-6591). – ISBN 978-1-4020-8868-1. – URL: http://dx.doi.org/10.1007/978-1-4020-8868-1 (дата обращения: 01.04.2022). – Access mode: for authorization. users.
Abstract: Provides and up to date review of the field. Each chapter presents research problems and contains a pedagogical component.
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