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White Dwarf Model Atmospheres: Synthetic Spectra for Supersoft Sources

Published online by Cambridge University Press:  17 January 2013

Thomas Rauch
Thomas Rauch*
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: rauch@astro.uni-tuebingen.de
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Abstract

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The Tübingen NLTE Model-Atmosphere Package (TMAP) calculates fully metal-line blanketed white dwarf model atmospheres and spectral energy distributions (SEDs) at a high level of sophistication. Such SEDs are easily accessible via the German Astrophysical Virtual Observatory (GAVO) service TheoSSA. We discuss applications of TMAP models to (pre) white dwarfs during the hottest stages of their stellar evolution, e.g. in the parameter range of novae and supersoft sources.

Keywords

astronomical data bases: miscellaneous — stars: abundancesAGB and post-AGBatmospheresearly-typeindividual (V 4743 Sgr, V 1974 Cyg)novaecataclysmic variableswindsoutflows — binaries: close — X-rays: binariesbursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 60 - 63
Copyright
Copyright © International Astronomical Union 2013

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