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Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl

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書目名稱Effects of Mass Loss on Stellar Evolution
副標(biāo)題IAU Colloquium no. 5
編輯C. Chiosi,R. Stalio
視頻videohttp://file.papertrans.cn/303/302865/302865.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl
描述The IAU Colloquium No. 59, "The effects of mass loss on Stellar Evolution" was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du- ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti- cal developments on the problem of mass loss from early ty- pe st
出版日期Book 1981
關(guān)鍵詞Accretion; Galaxy; star; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-8500-1
isbn_softcover978-94-009-8502-5
isbn_ebook978-94-009-8500-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1981
The information of publication is updating

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Book 1981related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti- cal developments on the problem of mass loss from early ty- pe st
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Summary, Conclusions, and Future Work,the WR mass loss may also be important for Of stars (Lamers 1980). A determination of the properties of the WR stellar winds will provide diagnostics which might aid in identifying the mass loss mechanism, and P-Cygni profiles form one important data source for this purpose. With the advent of IUE m
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An Introduction to Data Mining,± 100 km s.. Our preliminary evaluation of the associated mass loss rate gives 10. M. yr.. Other planetary nebulae nuclei are studied with low resolution IUE spectra and indications are found of mass loss rates consistent with the above value.
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