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- W2089699717 abstract "view Abstract Citations (53) References (13) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS On convective and semiconvective mixing in massive stars Cloutman, L. D. ; Whitaker, R. W. Abstract The evolutionary sequence of a 15.57-solar mass star made with a simplified turbulence transport model demonstrates the importance of accurately modeling the turbulent convection in the stellar interior. The combination of the self-diffusion of turbulence and its finite decay time in a stable region extend the convective core by about 3 solar masses, profoundly affecting the evolution of the star. Among the important effects are the elimination of semiconvection and the increase in both the lifetime and luminosity in the hydrogen-burning phase. Publication: The Astrophysical Journal Pub Date: May 1980 DOI: 10.1086/157937 Bibcode: 1980ApJ...237..900C Keywords: Main Sequence Stars; Stellar Evolution; Stellar Mass; Supermassive Stars; Convection; Statistical Analysis; Stellar Interiors; Stellar Luminosity; Stellar Models; Turbulence Effects; Astrophysics full text sources ADS |" @default.
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- W2089699717 date "1980-05-01" @default.
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- W2089699717 title "On convective and semiconvective mixing in massive stars" @default.
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