An improved set of radiation hydrodynamic equations for stellar oscillation

Details An improved set of radiation hydrodynamic equations for stellar oscillation An improved set of radiation hydrodynamic equations for stellar oscillation

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..300x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 3, p. 300-308.

Astronomy and Astrophysics

Astrophysics

Radiation, Convection, Hydrodynamics

Scientific paper

The set of hydrodynamic equations including radiation developed by the present author is refined in this paper. In the new formulation, the thermodynamic variables for matter and radiation are completely separated. This means not only greater internal consistency in the theory but also convenience in theoretical calculations of stellar pulsation. The new dynamic equations of turbulent convection are shown to be consistent with the previous ones.

Affiliated with

Also associated with

No associations

Rating

An improved set of radiation hydrodynamic equations for stellar oscillation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with An improved set of radiation hydrodynamic equations for stellar oscillation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An improved set of radiation hydrodynamic equations for stellar oscillation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1253875