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- W1971863221 abstract "Blue stragglers produced from physical stellar collisions are expected to be born rotating rapidly, while the blue stragglers observed in intermediate-age and old star clusters do not. We suggest that the collision and merger of two main-sequence stars results in an object that quickly swells into a pre-main-sequence-like star with a convective envelope, which can spin down via magnetic braking as it approaches its thermal equilibrium configuration. The result is a blue straggler with a rotation similar to that of a normal star of the same mass and age. Consequently, rapid rotation is not a signature of a collisionally merged blue straggler." @default.
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- W1971863221 date "1995-07-10" @default.
- W1971863221 modified "2023-10-12" @default.
- W1971863221 title "The Rotational Rates of Blue Stragglers Produced by Physical Stellar Collisions" @default.
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- W1971863221 doi "https://doi.org/10.1086/309581" @default.
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