A computer program for calculating non-LTE model stellar atmospheres

Details A computer program for calculating non-LTE model stellar atmospheres A computer program for calculating non-LTE model stellar atmospheres

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cophc..52..103h&link_type=abstract

Computer Physics Communications, Volume 52, Issue 1, p. 103-132.

Physics

475

Scientific paper

The program calculates model stellar atmospheres, assuming plane-parallel, horizontally homogeneous atmosphere in radiative and hydrostatic equilibrium, and allowing for departures from local thermodynamic equilibrium (LTE) for a set of occupation numbers of selected atomic and ionic energy levels. The program is very flexible as to the choice of chemical.

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