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• W3103820249 abstract "We explore the evolution of collisionally merged stars in the blue straggler region of the H-R diagram. The starting models for our stellar evolution calculations are the results of the smoothed particle hydrodynamics (SPH) simulations of parabolic collisions between main-sequence stars performed by Lombardi, Rasio, & Shapiro. Since SPH and stellar evolution codes employ different and often contradictory approximations, it is necessary to treat the evolution of these products carefully. The mixture and disparity of the relevant timescales (hydrodynamic, thermal relaxation, and nuclear burning) and of the important physical assumptions between the codes makes the combined analysis of the problem challenging, especially during the initial thermal relaxation of the star. In particular, the treatment of convection is important and semiconvection must be modeled in some detail." @default.
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• W3103820249 date "1997-09-20" @default.
• W3103820249 modified "2023-09-29" @default.
• W3103820249 title "Evolution of Stellar Collision Products in Globular Clusters. I. Head‐on Collisions" @default.
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• W3103820249 doi "https://doi.org/10.1086/304588" @default.
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