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Titlebook: Radio Stars; Proceedings of a Wor Robert M. Hjellming,David M. Gibson Conference proceedings 1985 D. Reidel Publishing Company, Dordrecht,

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書(shū)目名稱(chēng)Radio Stars
副標(biāo)題Proceedings of a Wor
編輯Robert M. Hjellming,David M. Gibson
視頻videohttp://file.papertrans.cn/821/820650/820650.mp4
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Radio Stars; Proceedings of a Wor Robert M. Hjellming,David M. Gibson Conference proceedings 1985 D. Reidel Publishing Company, Dordrecht,
描述This book is the proceedings of a workshop on stellar continuum radio astronomy that was held in BoUlder, Colorado on August 8-10, 1984. Although it was originally intended to be a small workshop with participants mainly from North America, it evolved to a workshop with 72 partiCipants from twelve countries (U.S.A. 52, Canada 3, the Netherlands 3, United Kingdom 3, Australia 2, Ireland 2, Italy 2, France 1, Mexico 1, Switzerland 1, West Germany 1, and U.S.S.R. 1). This workshop was sponsored by the Joint Institute of Laboratory Astrophysics (JILA) and the University of Colorado. In order to preserve a workshop atmosphere, while still presenting both extensive reviews and contributed papers, an experimental format was adopted. All contributed papers related to the topiCS of the day were presented in poster form in the early morning and were accessible all day. During each morning (or afternoon) session review papers were presented, followed by a coffee break in the poster area adjacent to the conference room. Then the review papers and contributed papers were discussed for roughly one and a half hours. The last session was devoted to invited panel papers and discussion of current an
出版日期Conference proceedings 1985
關(guān)鍵詞Accretion; astronomy; relativistic jet; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-5420-5
isbn_softcover978-94-010-8892-3
isbn_ebook978-94-009-5420-5Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1985
The information of publication is updating

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Damping of the Magnetoionic Z Modend, by analogy, in stellar radio sources also. In particular, we wish to know if a high z-mode energy density leads to observable radiation. We consider two effects here: damping of the z-mode waves as they propagate through the ambient coronal plasma, and coalescence of z-mode waves to produce seco
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Conference proceedings 1985rnoon) session review papers were presented, followed by a coffee break in the poster area adjacent to the conference room. Then the review papers and contributed papers were discussed for roughly one and a half hours. The last session was devoted to invited panel papers and discussion of current an
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