A SET OF THE IMPROVED RADIATION-HYDRODYNAMIC EQUATIONS FOR STELLAR OSCILLATIONS
Xiong Da-run(Purple Mountain Astronomical Observatory, Academic Sinica, Nanjing 210008)
The radiation-hydrodynamic quations for stellar oscillations developed in our earlier paper are refined. The variables describing the gas are separated from the radiative ones, that brings convenience for the numerical calculations of stellar oscillations. It is proved that the new dynamic equations of turbulent convection are consistent with the previous ones.