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Characteristics of convection and overshooting in RGB and AGB stars
RGB and AGB stars: convection of stars: turbulent convection model: con-vective overshooting
2011/9/28
Based on the turbulent convection model (TCM) of Li & Yang (2007), we have studied the characteristics of turbulent convection in the envelopes of 2 and 5M stars at the RGB and AGB phases. The TCM has...
SOME THREE-PARAMETER RELATIONS FOR PHYSICAL CHARACTERISTICS OF STARS
PHYSICAL CHARACTERISTICS STARS
2009/4/8
For homologous stars with μ(ρ, T ) the L-M-Te relation is derived
and tested against an observational material for the main-sequence stars. The transformations
comprising the radius and the surface ...