Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..461j&link_type=abstract
Chinese Astronomy and Astrophysics, Volume 21, Issue 4, p. 461-473.
Astronomy and Astrophysics
Astrophysics
3
Scientific paper
Using the mixing length theory we give expressions for turbulence pressure and the equation of state and various thermodynamic quantities when turbulence is included. On this basis we examined the size of turbulence in the evolution of two stars of masses 2.8 and 7.0 Msolar from the main sequence to the red giant and the AGB stages, Our results show that in the late stages the turbulence pressure near the surface of the star can be as much as 30% of the total pressure.
Huang Run-Qian
Jiang Su-Yun
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