Model atmospheres of R CrB stars

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

A procedure for computing model atmospheres of R CrB stars is discussed. The procedure is implemented in the SAM941 program, which is a modification of ATLAS9. Model atmospheres of the Sun and R CrB computed by using the MARCS and SAM941 programs are compared. The effect of various opacity sources on model atmospheres and emergent fluxes is studied. The dependences of the structure of R CrB model atmospheres on hydrogen and carbon abundances are shown to differ markedly.

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