On the local theory of stellar convection with μ-gradient using one-point correlation functions

Details On the local theory of stellar convection with μ-gradient using one-point correlation functions On the local theory of stellar convection with μ-gradient using one-point correlation functions

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mnras.391.1327u&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 391, Issue 3, pp. 1327-1331.

Astronomy and Astrophysics

Astronomy

Stars: Interiors

Scientific paper

The local equations of Xiong's theory of convection with one-point correlation functions contain the equations for an extended mixing length theory of convection with helium flux by Umezu & Nakakita. The equations also contain the equations for overstable convection of Kato. Similar equations can be derived from those of Grossman et al. and Canuto. The local convection and the overstable convection can be treated in a unified way with their localized equations.

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