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Titlebook: Stellar Nucleosynthesis; Proceedings of the T Cesare Chiosi,Alvio Renzini Conference proceedings 1984 D. Reidel Publishing Company, Dordrec

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书目名称Stellar Nucleosynthesis
副标题Proceedings of the T
编辑Cesare Chiosi,Alvio Renzini
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Stellar Nucleosynthesis; Proceedings of the T Cesare Chiosi,Alvio Renzini Conference proceedings 1984 D. Reidel Publishing Company, Dordrec
描述x about a sequence of reVlew lectures, each followed by contributed talks and discussions. The opening session was devoted to reviewing the most recent results concerning the determination of chemical abundances in particularly inte­ resting objects providing direct evidence for stellar nucleosynthesis (like planetary nebulae, supernovae and supernova remnants). In Session 2 recent results on some relevant nuclear reaction rates have been presented. Session 3 grouped the contributions concerning the quasi-static evolution of normal stars, its relevance for the nucleosynthesis of the varlOUS elements and isotopes, and the comparison of the evolutionary models with the observations. Session 4 addressed the important questions of identifying the precursors of both Type I and Type II supernovae, and of determining the detailed composition of the ejecta by explosive nucleosynthesis associated with these events. Finally, Session 5 was devoted to a presentation of recent calculations of the evolution of hypothetical pre-galactic very massive objects (in­ cluding their potential role in pre-galactic nucleosynthesis), and to reviewing the progress that has been made in understanding the che
出版日期Conference proceedings 1984
关键词Galaxy; Supernova; astronomy; cosmic ray; galaxies; planet; star; stars; stellar; stellar evolution; universe
版次1
doihttps://doi.org/10.1007/978-94-009-6348-1
isbn_softcover978-94-009-6350-4
isbn_ebook978-94-009-6348-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1984
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书目名称Stellar Nucleosynthesis影响因子(影响力)




书目名称Stellar Nucleosynthesis影响因子(影响力)学科排名




书目名称Stellar Nucleosynthesis网络公开度




书目名称Stellar Nucleosynthesis网络公开度学科排名




书目名称Stellar Nucleosynthesis被引频次




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书目名称Stellar Nucleosynthesis年度引用




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书目名称Stellar Nucleosynthesis读者反馈




书目名称Stellar Nucleosynthesis读者反馈学科排名




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Extragalactic Supernovaeout a century ago, when S Andromedae, now known also as SN 1885a, appeared near the nucleus of the Andromeda Galaxy. Fifty years later, after only 13 more SNe had been noticed, Zwicky appeared and the discovery rate rose sharply; the total number now exceeds 500. Detailed theoretical discussions of
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Abundances in Supernova Remnantsf nucleosynthesis and their contribution to metal enrichment in our galaxy. Very little of what I describe here is new but some of it is still in press and therefore relatively unknown. Many of the comments, particularly those on the optical properties, have been made in other contributions by Danzi
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A Statistical Comparison of Galactic SNRs and Galactic Giant HII Regions in longitude of 138 SNRs and 100 giant HII regions are presented, and compared with a simple Monte Carlo model in which 140 supernovae are distributed either along arms according to a density wave model, or uniformly in the plane. The model is intended to give a statistical measure of the ratio of
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Wolf — Rayet Stars, Cosmic Rays and Gamma Rayshe origin and acceleration of the cosmic radiation. It is shown that carbon rich Wolf-Rayet stars could play the role of auxiliary sources of cosmic rays, accelerating to relativistic energies the products of their nucleosynthesis (.C, .O, .Ne, .Mg, .Mg, .S, .Fe, s-process elements up to mass 90).Th
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Nuclear Effective Forces and their Use in Astrophysical Problems the same conviction. The success of phenomeno-logical, easy-to-use, formulae based on popular macroscopic theories may explain this self-confident attitude. Many astrophysical processes however deal with physical conditions or quantities which are not at present, and some will never be, accessible
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