| 书目名称 | Dynamics of Star Clusters | | 副标题 | Proceeding of the 11 | | 编辑 | Jeremy Goodman,Piet Hut | | 视频video | | | 丛书名称 | International Astronomical Union Symposia | | 图书封面 |  | | 描述 | The emphasis in these proceedings of lAD Symposium No. 113, Dynafrri-,‘!s of Star Clusters. and·.~.Le. mab rPIHlon for orZ‘lnizinp: thE" symposium in the spring of 1984, was the rapid increase during the preceeding year in our understanding of core collapse. The last I.A.D. Symposium to discuss the dynamics of star clusters at length was No.69, Dynamics of Stellar Systems~ held in Besan~on in 1974. For a few years afterwards, globular clusters receiveu much attention due to the discovery of X-ray bursters and the mounting evidence that X-ray sources in globular clusters were formed in completely different ways than those within our galaxy. Globular clusters, which until this time had a reputation for sedate old age, turned out to lead violent private lives at high energies. However, in the early 80‘s globular clusters seemed to lose some of the glamor of the 70‘s. The grand speculations of heavy black holes lurking in their centers had to make way for a variety of observational evidence which indicated that the X-ray sources are low-mass close binaries instead. But, though dynamical fashion turned to heavy galac tic halos and so on, some of the unsolved theoretical problems regard | | 出版日期 | Conference proceedings 1985 | | 关键词 | CCD; Galaxy; black hole; photometry; star; stellar; telescope | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-009-5335-2 | | isbn_softcover | 978-90-277-1965-2 | | isbn_ebook | 978-94-009-5335-2Series ISSN 1743-9213 Series E-ISSN 2352-2186 | | issn_series | 1743-9213 | | copyright | International Astronomical Union 1985 |
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发表于 2025-3-21 16:07:50
