Convection in Stellar Evolution Models

Details Convection in Stellar Evolution Models Convection in Stellar Evolution Models

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..948...87s&link_type=abstract

UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP Conference Proceedings, Volume 948, pp. 87-98

Physics

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Thermodynamic Processes, Conduction, Convection, Equations Of State

Scientific paper

The treatment of convection in stellar evolution calculations is briefly discussed, with emphasis on the modelling of low- and intermediate-mass stars. The specific cases of core convection during the central He-burning phase and surface superadiabatic convection are analyzed in more detail, as examples of the uncertainties involved in modelling convective regions within the current generation of stellar evolution codes.

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