Mass dependence of convective core overshooting in the low-intermediate mass stars

Details Mass dependence of convective core overshooting in the low-intermediate mass stars Mass dependence of convective core overshooting in the low-intermediate mass stars

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.276.1287u&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 276, Issue 4, pp. 1287-1294.

Astronomy and Astrophysics

Astronomy

10

Convection, Stars: Interiors

Scientific paper

Several authors have indicated that convective overshooting is very small for stars in the mass range of approximately 1.1-1.6M_solar, although these authors insist that larger overshooting occurs in more massive stars. In this paper, it is indicated that this small extent of convective core overshooting can be accounted for by using the non-local mixing length theory in conjunction with the turbulent viscous dissipation.

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