Theoretical White Dwarf Spectra on Demand: TheoSSA

Details Theoretical White Dwarf Spectra on Demand: TheoSSA Theoretical White Dwarf Spectra on Demand: TheoSSA

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..121r&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 121-124 (2010).

Astronomy and Astrophysics

Astrophysics

White Dwarfs, Spectral Analysis, Element Relative Abundance, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Spectroscopy And Spectrophotometry, Origin, Formation, And Abundances Of The Elements

Scientific paper

In the last decades, a lot of progress was made in spectral analysis. The quality (e.g. resolution, S/N ratio) of observed spectra has improved much and several model-atmosphere codes were developed. One of these is the ``Tübingen NLTE Model-Atmosphere Package'' (TMAP), that is a highly developed program for the calculation of model atmospheres of hot, compact objects.
In the framework of the German Astrophysical Virtual Observatory (GAVO), theoretical spectral energy distributions (SEDs) can be downloaded via TheoSSA. In a pilot phase, TheoSSA is based on TMAP model atmospheres. We present the current state of this VO service.

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