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Modelling of the spectra and atmospheres of evolved stars

Yakiv V. Pavlenko
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Abstract

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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Yakiv V. Pavlenko. 2006-06-11. Modelling of the spectra and atmospheres of evolved stars. https://arxiv.org/abs/astro-ph/0606252

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