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Titlebook: Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation; Proceedings of the E Lex Kaper,Edward P. J. van den Heu

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發(fā)表于 2025-3-21 19:54:17 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation
期刊簡稱Proceedings of the E
影響因子2023Lex Kaper,Edward P. J. van den Heuvel,Patrick A. W
視頻videohttp://file.papertrans.cn/189/188947/188947.mp4
學科分類ESO Astrophysics Symposia
圖書封面Titlebook: Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation; Proceedings of the E Lex Kaper,Edward P. J. van den Heu
影響因子The observational evidence for the existence of black holes has grown significantly over recent decades. Stellar-mass black holes are detected as X-ray sources in binary systems, while supermassive black holes, with masses more than a million times the mass of the Sun, lurk in the nuclei of galaxies. These proceedings provide a useful and up-to-date overview of the observations of black holes in binaries, in the center of the Milky Way, and in the nuclei of galaxies, presented by leading expert astronomers. Special attention is given to the formation (including the recent evidence from gamma-ray bursts), physical properties, and demographics of black holes.
Pindex Conference proceedings 2001
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,Theorien zu Unternehmensübernahmen,ll stellar motions are very close to isotropy. They indicate a central mass concentration with a density . M. pc. that dominates the potential between 0.01 and 1 pc. The derived mass ranges between 2.6 and 3.3 x 10. M. for a distance of 8.0 kpc. Such a mass concentration cannot be stable and must be
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Hans-Gert Penzel,Christian PietigThe maximum mass of neutron stars is one of the most important predictions of the general relativistic theory of stellar structure. This paper highlights the difficulties in making a definitive prediction, and also reviews the progress made so far.
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David Fubini,Colin Price,Maurizio ZolloThe advent of the large effective apertures of the Keck telescopes has resulted in the determination with unprecedented accuracy of the mass functions and mass ratios of faint (. mag) X-ray transients (GS 2000+25, GRO J0422+32, Nova Oph 1977, Nova Vel 1993).
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