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Titlebook: Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion; Proceedings of the 1 Ken‘ichi Nomoto Conferen

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期刊全稱Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion
期刊簡(jiǎn)稱Proceedings of the 1
影響因子2023Ken‘ichi Nomoto
視頻videohttp://file.papertrans.cn/165/164616/164616.mp4
學(xué)科分類Lecture Notes in Physics
圖書封面Titlebook: Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion; Proceedings of the 1 Ken‘ichi Nomoto Conferen
影響因子This collection of papers describes the evolutionary path of stars of various masses. Observational data and theoretical modeling of the stellar atmosphere and the stellar interior and their interaction are presented, covering chemical peculiarities, mass loss, and explosion, all of which are strongly related to the hydrodynamic evolution of the interior. In particular the supernova SN 1987 A is discussed for the first time in detail, including the underground neutrino observations and the detection of X-rays from the supernova. The study of its progenitor, a B 3 supergiant, was related to the topics of chemical peculiarities and mass loss mechanisms and atmospheric models. The intended readers are professional astronomers and astrophysicists, as well as physicists. The book will also be an important source of information for graduate students.
Pindex Conference proceedings 1988
The information of publication is updating

書目名稱Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion影響因子(影響力)




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https://doi.org/10.1007/BFb0034541Accretion; Anomalie; LOPES; Superhump; Supernova; atmosphere; evolution; gravity; paper; planet; spectroscopy;
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978-3-662-13701-7Springer-Verlag Berlin Heidelberg 1988
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0075-8450 llar atmosphere and the stellar interior and their interaction are presented, covering chemical peculiarities, mass loss, and explosion, all of which are strongly related to the hydrodynamic evolution of the interior. In particular the supernova SN 1987 A is discussed for the first time in detail, i
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