| 書目名稱 | Short-Period Binary Stars: Observations, Analyses, and Results | | 編輯 | Eugene F. Milone,Denis A. Leahy,David W. Hobill | | 視頻video | http://file.papertrans.cn/867/866741/866741.mp4 | | 概述 | The observational techniques include gravitational wave investigations, X-ray, radio, infrared, and optical astronomy; and the ways in which these objects are analyzed.Among the specific objects repor | | 叢書名稱 | Astrophysics and Space Science Library | | 圖書封面 |  | | 描述 | .Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. These objects represent stages of evolution of binary stars, and their degrees of separation provide critical clues to how their evolutionary paths differ from that of single stars. The widest and least distorted systems provide astronomers with the essential precise data needed to study all stars: mass and radius. The interactions of binary star components, on the other hand, provide a natural laboratory to observe how the matter in these stars behaves under different and often varying physical conditions. Thus, cataclysmic variables with and without overpoweringly strong magnetic fields, and stars with densities from that found in the Sun to the degenerate matter of white dwarfs and the ultra-compact states of neutron stars and black holes are all discussed. The extensive index permits cross-referencing.. | | 出版日期 | Book 2008 | | 關鍵詞 | Accretion; Interacting binaries; X-ray binaries; astronomy; astrophysics; black holes; cataclysmic variabl | | 版次 | 1 | | doi | https://doi.org/10.1007/978-1-4020-6544-6 | | isbn_softcover | 978-90-481-7666-3 | | isbn_ebook | 978-1-4020-6544-6Series ISSN 0067-0057 Series E-ISSN 2214-7985 | | issn_series | 0067-0057 | | copyright | Springer Science+Business Media B.V. 2008 |
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