Statistics – Computation
Scientific paper
Sep 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.252...56u&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 252, Sept. 1, 1991, p. 56-62.
Statistics
Computation
6
Computational Astrophysics, Convective Heat Transfer, Helium, Massive Stars, Radiative Heat Transfer, Stellar Cores, Heat Flux, Mathematical Models, Mixing Length Flow Theory, Temperature Gradients
Scientific paper
The nonlocal mixing-length theory of stellar convective cores by Maeder is extended to include the effects of radiative heat loss from the convective element, and of helium flux. The radiative heat loss tends to enlarge the overshooting region, although it barely changes the size of the overshooting core for the ordinarily accepted size of the convective element. The helium gradient seems negligible in the overshooting region.
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