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Titlebook: Neutron Stars, Black Holes and Binary X-Ray Sources; Herbert Gursky,Remo Ruffini Book 1975 Springer Science+Business Media Dordrecht 1975

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发表于 2025-3-21 19:28:28 | 显示全部楼层 |阅读模式
书目名称Neutron Stars, Black Holes and Binary X-Ray Sources
编辑Herbert Gursky,Remo Ruffini
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Neutron Stars, Black Holes and Binary X-Ray Sources;  Herbert Gursky,Remo Ruffini Book 1975 Springer Science+Business Media Dordrecht 1975
描述This book contains a set of articles based on a session of the annual meeting of the American Association for the Advancement of Science held in San Francisco in February, 1974. The reason for the meeting arose from the need to communicate to the largest possible scientific community the dramatic advances which have been made in recent years in the understanding of collapsed objects: neutron stars and black holes. Thanks to an unprecedented resonance between X-ray, y-ray, radio and optical astronomy and important new theoretical developments in relativistic astro­ physics, a new deep understanding has been acquired of the physical processes oc­ curring in the late stages of evolution of stars. This knowledge may be one of the greatest conquests of man‘s understanding of nature in this century. This book aims to give an essential and up-to-date view in this field. The analysis of the physics and astrophysics of neutron stars and black holes is here attacked from both theoretical and experimental points of view. In the experimental field we range from the reviews and catalogues of galactic X-ray sources (R. Gursky and E. Schreier) and pulsars (E. Groth) to the observations of the opt
出版日期Book 1975
关键词Accretion; Supernova; astronomy; astrophysics; black hole; black holes; cosmic ray; gamma-ray burst; gravita
版次1
doihttps://doi.org/10.1007/978-94-010-1767-1
isbn_softcover978-90-277-0542-6
isbn_ebook978-94-010-1767-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1975
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发表于 2025-3-21 20:57:29 | 显示全部楼层
Observational Properties of Pulsars,een learned of their properties. Pulsars are slowly rotating (~1 Hz) neutron stars with huge magnetic fields (~10. G) which convert rotational energy into energy of (radio) radiation and relativistic particles. The pulsed radiation presumably arises from a beaming effect associated with the magnetic field.
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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/n/image/664686.jpg
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https://doi.org/10.1007/978-94-010-1767-1Accretion; Supernova; astronomy; astrophysics; black hole; black holes; cosmic ray; gamma-ray burst; gravita
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iert worden. Nun stellt sich mit dieser Diagnose vor Augen abschließend die Frage: Was ist angesichts der gefundenen Probleme zu tun? Oder erst einmal allgemeiner: Ist überhaupt etwas zu tun? Es gibt nicht wenige Stimmen, die vor einer herbeigeredeten Dramatik warnen und darauf hinweisen, daß ein un
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Herbert Gursky,Remo Ruffinie in Nordamerika deuten auf einen sich weltweit abzeichnenden Trend einer Regionali-sierung der internationalen wirtschaftlichen Beziehungen hin. USA, Europa und Japan als wirtschaftliche Gravitationszentren für die umgebenden Regionen stellen die bedeutendsten Weltwirtschaftsregionen dar. Diese “Tr
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Stirling A. Colgateten Standortes für seine marketing-strategische Bearbeitung geben. Zunächst stellt sich die Notwendigkeit der räumlichen Eingrenzung des betrachteten Raumes. Innerhalb dieser Abgrenzung soll anschließend die Vielfalt der Marktregion in natur- und kulturgeographischer sowie in wirtschaftlicher Hinsic
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