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- W2963953908 abstract "Massive stars becoming red supergiants lose a significant amount of their mass during that brief evolutionary phase. They then either explode as a hydrogen-rich supernova (SN Type II), or continue to evolve as a hotter supergiant (before exploding). The slow, dusty ejecta of the red supergiant will be over-run by the hot star wind and/or SN ejecta. I will present estimates of the conditions for this interaction and discuss some of the implications." @default.
- W2963953908 created "2019-07-30" @default.
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- W2963953908 date "2009-06-26" @default.
- W2963953908 modified "2023-10-17" @default.
- W2963953908 title "The effects of red supergiant mass loss on supernova ejecta and the circumburst medium" @default.
- W2963953908 hasPublicationYear "2009" @default.
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