Poster abstract details
Spectral Analysis with the Virtual Observatory Tool TheoSSA
Abstract
In the framework of a German Astrophysical Virtual Observatory (GAVO)
project spectral energy distributions for the analysis of hot objects
like central stars of planetary nebulae were made accessible by the
service TheoSSA.
By now this service is based on the Tübingen NLTE Model-Atmosphere
Package TMAP, a code developed and tested over the last 25 years.
We present the possibilities of TheoSSA comparing the service
results with ``classical'' spectral analyses of the DO white dwarf and
central star of a planetary nebula PG1034+001.
project spectral energy distributions for the analysis of hot objects
like central stars of planetary nebulae were made accessible by the
service TheoSSA.
By now this service is based on the Tübingen NLTE Model-Atmosphere
Package TMAP, a code developed and tested over the last 25 years.
We present the possibilities of TheoSSA comparing the service
results with ``classical'' spectral analyses of the DO white dwarf and
central star of a planetary nebula PG1034+001.