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Titlebook: Late Stages of Stellar Evolution; R. J. Tayler,J. E. Hesser Book 1974 International Astronomical Union 1974 gravitation.gravity.planet.sta

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书目名称Late Stages of Stellar Evolution
编辑R. J. Tayler,J. E. Hesser
视频video
丛书名称International Astronomical Union Symposia
图书封面Titlebook: Late Stages of Stellar Evolution;  R. J. Tayler,J. E. Hesser Book 1974 International Astronomical Union 1974 gravitation.gravity.planet.sta
描述lAD Symposium No. 66 was held in Warsaw from September 10th to September 12th 1973, in connection with the Extraordinary General Assembly of the lAD. It was arranged by lAD Symposium No. 35 and the Scientific Organising Committee con­ sisted of A. G. Massevitch (Chairman), A. V. Tutukov (Secretary), H. M. van Horn, N. Dallaporta, J. P. Ostriker, B. Paczynski, G. Ruben, E. Schatzman, R. J. Tayler and A. Weigert. This volume contains the full texts of all of the invited papers presented at the Symposium, apart from that delivered by R. P. Kraft, which is published in abstract because it is appearing in full elsewhere. In addition the short communications given at the Symposium are published in abstract. I attempted to take down all of the dis­ cussion as it occurred and all contributors to the discussion were asked to provide copies of their remarks. From these sources an edited version of the discussion has been produced. As the final version has not been seen by the contributors, I should be held responsible for all errors. At Warsaw, some of the short communications did not immediately follow the invited paper to which they referred. In the printed version they and any discussion
出版日期Book 1974
关键词gravitation; gravity; planet; star; stellar; stellar evolution; sun
版次1
doihttps://doi.org/10.1007/978-94-010-2237-8
isbn_softcover978-90-277-0471-9
isbn_ebook978-94-010-2237-8Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1974
The information of publication is updating

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Late Stages of Stellar Evolution978-94-010-2237-8Series ISSN 1743-9213 Series E-ISSN 2352-2186
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International Astronomical Union Symposiahttp://image.papertrans.cn/l/image/581781.jpg
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Mass Ejection by Radiation Pressure, the optically thick regions. There were many attempts to find selfconsistent models of time-independent mass outflow driven by this mechanism (Finzi and Wolf, 1971; Bisnovaty-Kogan and Nadyozhin, 1972; and many others); however, neither was satisfactory.
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Nuclear Reactions and Neutrinos in Stellar Evolution,Much of the material discussed in this review represents a summary of some chapters in a monograph I am writing (Arnett, 1974); a more detailed discussion will be found there.
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Non-Explosive Mass Loss,The various mechanisms whereby stars might lose matter are considered, together with the observational evidence of the mass loss rates associated with these mechanisms. The results are shown in a diagram giving the fractional mass that a star loses by various mechanisms as a function of initial mass.
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