Abstract
The problem of modeling the convection in red giant envelopes is addressed with two-dimensional nonlinear and nonadiabatic simulations. Hydrostatic envelopes, in thermal equilibrium, were integrated using the mixing-length theory (MLT) for different values of the mixing-length parameter λ. We examined the energy balance for two-dimensional simulations by using the MLT envelopes as initial model. On the basis of these two-dimensional simulations, we identify a model that is close to two-dimensional equilibrium. Such a model is characterized by an initial mixing-length parameter. Its value depends upon the numerical resolution, varying from 1.0 for low resolution to 1.5 for the best resolution at present.
Original language | English |
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Pages (from-to) | L47-L50 |
Journal | Astrophysical Journal |
Volume | 491 |
Issue number | 1 PART II |
DOIs | |
State | Published - 1997 |
Keywords
- Convection
- Methods: numerical
- Stars: AGB and post-AGB
- Stars: atmospheres