Stellar Turbulent Convection. I. Theory-Reference-Cited by-同舟云学术

Stellar Turbulent Convection. I. Theory

Published:1998-02 Issue:2 Volume:493 Page:834-847
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Canuto V. M.,Dubovikov M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/493/i=2/a=834/pdf

Reference65 articles.

1. Evolution of DB white dwarfs in the Canuto and Mazzitelli theory of convection

2. New strong evidence for the importance of convective overshooting in intermediate-mass stars

3. Antia, H. M. & Basu, S. 1997, in Solar Convection, Oscillations and their Relationship, SCORE 1996, ed. F. P. Pijpers, J. Christensen-Dalsgaard, & C. S. Rosenthal (Dordrecht: Kluwer)

4. Solar pulsational stability - I. Pulsation-mode thermodynamics

5. Seismology of the base of the solar convection zone

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