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- W3100926460 abstract "Abstract The progenitors of many core-collapse supernovae (CCSNe) are expected to be in binary systems. By performing a series of three-dimensional hydrodynamical simulations, we investigate how CCSN explosions affect their binary companion. We find that the amount of removed stellar mass, the resulting impact velocity, and the chemical contamination of the companion that results from the impact of the SN ejecta, strongly increases with decreasing binary separation and increasing explosion energy. Also, it is foud that the impact effects of CCSN ejecta on the structure of main-sequence (MS) companions, and thus their long term post-explosion evolution, are in general not dramatic." @default.
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- W3100926460 date "2018-08-01" @default.
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- W3100926460 title "The interaction of core-collapse supernova ejecta with a stellar companion" @default.
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- W3100926460 doi "https://doi.org/10.1017/s1743921318007913" @default.
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