Paper:	Model Atmospheres and Spectra of Peculiar Stars
Volume:	401, RS Ophiuchi (2006) and the Recurrent Nova Phenomenon
Page:	124
Authors:	Pavlenko, Y.V.; Evans, A.; Duerbeck, H.W.; Geballe, T.; Yakovina, L.; Kaminsky, B.; Kerr, T.
Abstract:	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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