Abstract
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. Copyright © International Astronomical Union 2013.
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CITATION STYLE
Rauch, T. (2013). White dwarf model atmospheres: Synthetic spectra for supersoft sources. In Proceedings of the International Astronomical Union (Vol. 7, pp. 60–63). Cambridge University Press. https://doi.org/10.1017/S174392131201469X
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