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Titlebook: Double Stars, Physical Properties and Generic Relations; Proceeding of IAU Co Bambang Hidayat,Zdeněk Kopal,Jürgen Rahe Conference proceedin

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書目名稱Double Stars, Physical Properties and Generic Relations
副標題Proceeding of IAU Co
編輯Bambang Hidayat,Zdeněk Kopal,Jürgen Rahe
視頻videohttp://file.papertrans.cn/283/282691/282691.mp4
圖書封面Titlebook: Double Stars, Physical Properties and Generic Relations; Proceeding of IAU Co Bambang Hidayat,Zdeněk Kopal,Jürgen Rahe Conference proceedin
描述The Bosscha Observatory in Lembang, Java, Indonesia, celebrated in 1983 its 60th anniversary. Since its foundation, the physical properties of binary systems have formed a major research topic of this observatory. Until 1970, the study of visual binaries and the determination of orbits received most emphasis. Since then, also the evolution of close binary systems, such as X-ray binaries, Wolf-Rayet binaries and binary pulsars, has been researched with priority in Lembang. It seemed thus appropriate that a Colloquium devoted to the study of binary systems be held in Lembang at the time of the Observatory‘s anniversary. In the Colloquium, the role of wide double (and multiple) systems received special emphasis - not only because of the long tradition of visual binary research at Lembang; but also because their role in documenting stellar evolution has been largely overlooked in recent decades, and needs to be brought into focus with the information forthcoming from close binaries. The Colloquium covered the physical properties of visual as well as close binary systems, and their generic relations, in the broadest possible sense. It was sponsored by the International Astronomical Unio
出版日期Conference proceedings 1984
關(guān)鍵詞Galaxy; Variation; astronomy; galaxies; star; star formation; stellar; stellar evolution
版次1
doihttps://doi.org/10.1007/978-94-009-6372-6
isbn_softcover978-94-009-6374-0
isbn_ebook978-94-009-6372-6
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1984
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沙發(fā)
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https://doi.org/10.1007/978-981-15-5366-0star census for all kind of systems: close, medium, and wide. The Hipparcos satellite will probably add some important informations in that respect but ground-based observations also remain of the highest importance (radial velocities, photometry, astrometry, etc.).
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Madhumita Bandyopadhyay,Sunita Chughe speckle interferometric measurements of a sufficiently large sample of close visual binaries are suggested to settle this important observational question. The present paper is special in that it brings together a wealth of useful information, both observational and theoretical, in one place.
9#
發(fā)表于 2025-3-23 03:53:20 | 只看該作者
Sandeep Narula,Narma Bhattacharyartance, because it is only one of very few earlytype systems for which reliable limb-darkening coefficients can be expected to be obtained. The contribution of the light of the third component to the system has also been determined, and it appears most likely that VV Ori C is a star of spectral type A3 V.
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