A non-LTE model stellar atmosphere computer program

Computer Science

Scientific paper

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Atmospheric Models, Computer Programs, Early Stars, Stellar Atmospheres, Difference Equations, Equilibrium Equations, Hydrostatics, Linearization, Radiative Transfer, Stellar Radiation, Stellar Spectra, Transfer Functions

Scientific paper

A computer program was developed for calculating model atmospheres of
early-type stars subject to the constraints of radiative, hydrostatic,
and statistical equilibrium, by means of a complete-linearization
technique. This program is available through the NCAR High Altitude
Observatory's Radiative Transfer Library.

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