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Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra
ArticleAbstract: Aims. We present a database of 43 340 atmospheric models (∼80 000 models at the conclusion of the prPalabras claves:methods: data analysis, miscellaneous, Stars: atmospheresAutores:Arias L., Arrieta A., Fierro-Santillán C.R., Hareter M., Klapp J., Raul E. Puebla, Sigalotti L.D.G., Valencia J.M., Zsargó J.Fuentes: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:googlescopusX-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Crucis
ArticleAbstract: Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries inPalabras claves:accretion, accretion disks, Binaries: symbiotic, X-rays: binariesAutores:Cusumano G., Jaque Arancibia M., Lucy A.B., Luna G.J.M., Mukai K., Nelson T., Nuñez N.E., Raul E. Puebla, Segreto A., Sokoloski J.L., Walter F.Fuentes:googlescopus