Solution of the stellar structure equations in Eulerian coordinates

Details Solution of the stellar structure equations in Eulerian coordinates Solution of the stellar structure equations in Eulerian coordinates

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pasp...88..806d&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 88, Oct.-Nov. 1976, p. 806, 807. ERDA-supported research.

Astronomy and Astrophysics

Astronomy

1

Hydrostatics, Poisson Equation, Stellar Structure, Thermodynamic Equilibrium, Boundary Value Problems, Energy Transfer, Euler-Lagrange Equation, Finite Difference Theory, Lagrange Coordinates, Linear Equations, Radiative Transfer, Stellar Mass, Stellar Temperature

Scientific paper

The equations of hydrostatic and thermal equilibrium, assuming only radiative energy transport and spherical symmetry, are solved in Eulerian coordinates by a suitable modification of the Henyey method. An Eulerian approach may possibly be more suitably extended to more spatial dimensions than the usual Lagrangian procedure. The principle advantage of this method is that the equations of hydrostatic and thermal equilibrium and Poisson's equation may be solved simultaneously.

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