A Code for Calculating Static Model Stellar Atmospheres

Details A Code for Calculating Static Model Stellar Atmospheres A Code for Calculating Static Model Stellar Atmospheres

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jkas...42...47n&link_type=abstract

Journal of the Korean Astronomical Society, vol. 42, no. 3, pp. 47-54

Astronomy and Astrophysics

Astronomy

Stars: Stellar Atmosphere, Fundamental Parameters, Methods: Numerical

Scientific paper

In this paper we present an independent FORTRAN code for calculating LTE-plane-parallel model atmospheres. The transfer equation has been solved using Avrett and Loeser method. It is shown that, using an approximate non-gray temperature distribution together with the iteration
factors method (Simonneau and Crivellari) for correcting the temperature distribution reduce the number of iteration required to
achieve the condition of radiative equilibrium. Preliminary results for pure helium model atmospheres are presented.

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