headway
发表于 2025-3-25 07:00:24
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
大火
发表于 2025-3-25 08:36:18
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Acetaminophen
发表于 2025-3-25 12:54:51
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
lesion
发表于 2025-3-25 19:31:47
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
发表于 2025-3-25 22:44:35
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终止
发表于 2025-3-26 03:02:16
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slow-wave-sleep
发表于 2025-3-26 05:23:49
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培养
发表于 2025-3-26 12:08:55
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/v/image/982615.jpg
nonplus
发表于 2025-3-26 15:38:56
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
Peak-Bone-Mass
发表于 2025-3-26 17:28:49
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