Model Atmospheres and Spectra of Peculiar Stars

Statistics – Computation

Scientific paper

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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 and spectra are computed with special consideration of the particular problems encountered for peculiar and hydrogen deficient stars in the later stages of evolution. We present some computed model atmospheres and fits to observed spectra of Sakurai's object, V838 Mon, and RS Oph.

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