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Titlebook: Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments; Proceedings of IAU C H. Drechsel,Y. Kondo,J. Rahe

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書(shū)目名稱Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments
副標(biāo)題Proceedings of IAU C
編輯H. Drechsel,Y. Kondo,J. Rahe
視頻videohttp://file.papertrans.cn/223/222416/222416.mp4
圖書(shū)封面Titlebook: Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments; Proceedings of IAU C H. Drechsel,Y. Kondo,J. Rahe
描述Recent advances in observational and theoretical efforts in understanding the nature of cataclysmic variables had reached such maturity that there existed a strong, shared feeling among the workers in this field that an international colloquium sponsored by the International Astronomical Union would be timely. To be more specific, this was due primarily to the accumulation of the new data from satellite observatories, such as the International Ultraviolet Observatory (IUE) and EXOSAT, as well as ground-based optical and radio telescopes, and the advances in modeling the putative accretion disks and the thermo-nuclear run-away phenomena in the vinicity of the white dwarf stars in cataclysmic variables. A series of workshops on this subject held in North America over the past several years and that held in Europe in 1985 had all contributed to the advances in our knowledge that led to IAU Colloguium No. 93, held in Bamberg from the 16th to 19th of June 1986. In all, 157 astronomers from 27 countries participated in this conference. Judging from the papers presented, both invited and contributed, and from the enthusiasm seen in discussions, the meeting was indeed a success.
出版日期Conference proceedings 1987
關(guān)鍵詞CCD; Galaxy; accretion disk; observatory; photometry; planet; spectroscopy; star; stellar; telescope
版次1
doihttps://doi.org/10.1007/978-94-009-3801-4
isbn_softcover978-94-010-8191-7
isbn_ebook978-94-009-3801-4
copyrightSpringer Science+Business Media Dordrecht 1987
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Spectroscopy of the Primary and Secondary Components of the Dwarf Nova AH Herculisossible to calculate the relative contributions of the primary and secondary to the total light at the wavelength of Na D as a function of the exact spectral subtype of the secondary, using the measured equivalent width of the Na D lines. Taking the spectral gradient of primary and secondary from th
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Conference proceedings 1987Colloguium No. 93, held in Bamberg from the 16th to 19th of June 1986. In all, 157 astronomers from 27 countries participated in this conference. Judging from the papers presented, both invited and contributed, and from the enthusiasm seen in discussions, the meeting was indeed a success.
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Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments978-94-009-3801-4
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there existed a strong, shared feeling among the workers in this field that an international colloquium sponsored by the International Astronomical Union would be timely. To be more specific, this was due primarily to the accumulation of the new data from satellite observatories, such as the Intern
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