Modelling of the spectra and atmospheres of evolved stars

Details Modelling of the spectra and atmospheres of evolved stars Modelling of the spectra and atmospheres of evolved stars

2006-06-11

arxiv.org/abs/astro-ph/0606252v1

Mem.Soc.Ast.It. 75 (2004) 282

Astronomy and Astrophysics

Astrophysics

To be published in Memorie della Societa' Astronomica Italiana, as a contributed talk for the VIII Torino Workshop on Nucleosy

Scientific paper

The method and results of the computation of the model atmospheres and spectral energy distributions of chemically peculiar stars, are discussed. The models are computed with a special consideration of the particular problems encountered when computing model atmospheres for M and C-giants, and of hydrogen deficient stars. We present some computed model atmospheres for Sakurai's object, giants of globular clusters, and C-giants.

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