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- W3102571489 abstract "We use smoothed-particle hydrodynamics to examine differences between direct collisions of single stars and binary star mergers in their roles as possible blue straggler star formation mechanisms. From our simulations, we find in all cases that core helium in the progenitor stars is largely retained in the core of the remnant, almost independent of the type of interaction or the central concentration of the progenitor stars." @default.
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- W3102571489 date "1997-03-01" @default.
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- W3102571489 title "Composition Mixing during Blue Straggler Formation and Evolution" @default.
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- W3102571489 doi "https://doi.org/10.1086/303709" @default.
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