| 書目名稱 | Light Curve Modeling of Eclipsing Binary Stars | | 編輯 | E. F. Milone | | 視頻video | http://file.papertrans.cn/586/585986/585986.mp4 | | 圖書封面 |  | | 描述 | In the two decades since the development of the first eclipsing-binary modeling code, new analytic techniques and the availability of powerful, sometimes dedicated computing facilities have made possible vastly improved determinations of fundamental and even transient stellar parameters. The scale of these developments, of course, raises questions about modeling tools, techniques, and philosophies, such as: Who will maintain and upgrade the codes? Will the codes be open to improvement by outsiders, and if so, how? And, indeed, what should be the goals of a modeling program? Such questions had not been aired for a long time and, for this reason alone, deserved to be discussed in as general a forum as the community provides. This volume contains material presented by Commission 42 (Close Binary Stars) during the International Astronomical Union‘s XXI General Assembly in Argentina, July 1991, and during IAU Colloquium 151, Cordoba, Argentina, August 1991. The techniques discussed include simulations of stellar bright and dark spots, streams, partial and complete stellar disks, prominences, and other features characterizing active stars; modeling of polarization parameters; models that | | 出版日期 | Conference proceedings 1993 | | 關鍵詞 | Periastron; Variation; atmosphere; star; stellar | | 版次 | 1 | | doi | https://doi.org/10.1007/978-1-4612-2742-7 | | isbn_softcover | 978-1-4612-7649-4 | | isbn_ebook | 978-1-4612-2742-7 | | copyright | Springer-Verlag New York, Inc. 1993 |
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