White Dwarf Model Atmospheres: Synthetic Spectra for Super Soft Sources

Details White Dwarf Model Atmospheres: Synthetic Spectra for Super Soft Sources White Dwarf Model Atmospheres: Synthetic Spectra for Super Soft Sources

2011-08-31

arxiv.org/abs/1108.6168v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 2 figures

Scientific paper

The T\"ubingen 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 super soft sources.

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