Titlebook: Very Massive Stars in the Local Universe; Jorick S. Vink Book 2015 Springer International Publishing Switzerland 2015 100 Solar Mass Stars

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Evolution and Nucleosynthesis of Very Massive Stars, advanced phases of their evolution similar to stars with initial masses between 60 and 120?.. A distinctive feature which may be used to disentangle Wolf-Rayet stars originating from VMS from those originating from lower initial masses is the enhanced abundances of neon and magnesium at the surface

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0067-0057 ntroductory content for graduate (PhD) students and researchers from different branches of astronomy to be able to enter this exciting new field of very massive stars..978-3-319-34514-7978-3-319-09596-7Series ISSN 0067-0057 Series E-ISSN 2214-7985

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Mass-Loss Rates of Very Massive Stars,We discuss the basic physics of hot-star winds and we provide mass-loss rates for (very) massive stars. Whilst the emphasis is on theoretical concepts and line-force modelling, we also discuss the current state of observations and empirical modelling, and we address the issue of wind clumping.

臭名昭著

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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/v/image/982615.jpg

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https://doi.org/10.1007/978-3-319-09596-7100 Solar Mass Stars; Evolution of Very Massive Stars; Explosion of Very Massive Stars; Mass Loss of Ve

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