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A method for the study of accretion disk emission in cataclysmic variables. I. the model
ArticleAbstract: We have developed a spectrum synthesis method for modeling the ultraviolet (UV) emission from the acPalabras claves:accretion, accretion disks, Novae, cataclysmic variables, Stars: mass-loss, ultraviolet: generalAutores:Diaz M.P., Hubeny I., John Hillier D., Raul E. PueblaFuentes:googlescopusX-ray, UV and optical analysis of supergiants: ε Ori
ArticleAbstract: We present a multi-wavelength (X-ray to optical) analysis, based on non-local thermodynamic equilibrPalabras claves:Stars: abundances, Stars: individual: ε Ori, Stars: mass-loss, Stars: massive, Supergiants, Techniques: spectroscopicAutores:Cohen D.H., John Hillier D., Leutenegger M.A., Raul E. Puebla, Zsargó J.Fuentes:googlescopus