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Titlebook: Cataclysmic Variables and Low-Mass X-Ray Binaries; Proceedings of the 7 Donald Q. Lamb,Joseph Patterson Conference proceedings 1985 D. Reid

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书目名称Cataclysmic Variables and Low-Mass X-Ray Binaries
副标题Proceedings of the 7
编辑Donald Q. Lamb,Joseph Patterson
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Cataclysmic Variables and Low-Mass X-Ray Binaries; Proceedings of the 7 Donald Q. Lamb,Joseph Patterson Conference proceedings 1985 D. Reid
描述Since 1976 a meeting devoted to recent research on cataclysmic variables ("CV workshop") has been held annually somewhere in North America. Many of the meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi­ zing a meeting in Massachusetts in the middle of winter. Nobody wants their meeting to go down in history as the smallest and dullest, and it ~ surely be the coldest. But on occasion, meeting organizers have defied custom and scheduled meetings for less~than-trendy places, and gotten away with it (Ur·bana, IL and Rochester, NY must be reckoned as examples of this). Encouraged by the spatial and temporal proximity of the American Astronomical Society meeting (Boston, January 9-12), we thought we might get away with it again, and so came to organize a meeting for January 12-15, 1983, in Cambridge, MA. There was another reason for a meeting at this time and place, we loftily proclaimed in early mailings. No one doubts that the CV‘s are closely related to the low-mass X-ray binaries ("LMX
出版日期Conference proceedings 1985
关键词Accretion; Bulge; accretion disk; gravitation; gravity; neutron star; star; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-5319-2
isbn_softcover978-94-010-8849-7
isbn_ebook978-94-009-5319-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1985
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Abell 41, A Cataclysmic Variable Progenitorwith its critical Roche surface in the astronomically near future initiating mass transfer and cataclysmic activity..The existence of this star provides direct evidence for theoretical work suggesting that binary stars which, have suffered catastrophic angular momentum loss through the ejection of a
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Galactic Bulge X-Ray Burst Sources from Disrupted Globular Clusters ?.≲ 19) G or K star is found within the error circle (3″ radius) in four cases. These may be surviving giants in a disrupted globular cluster core. Implications for globular cluster evolution and the GXRBS themselves are discussed.
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