TMAW -- Tübingen Model Atmosphere Package WWW InterfaceTMAWivo://org.gavo.dc/theossa/q/tmawThe GAVO DC teamRauch, T.2022-01-13T13:38:11ZThomas Rauchgavo@listserv.uni-tuebingen.de++49 7071 2978614spectroscopyastronomical-simulationspost-asymptotic-giant-branch-starsstellar-atmospheres
The Tübingen NLTE Model-Atmosphere Package (`TMAP
<http://astro.uni-tuebingen.de/%7ETMAP/TMAP.html>`_) is a tool to calculate
stellar atmospheres in spherical or plane-parallel geometry in hydrostatic
and radiative equilibrium allowing departures from local thermodynamic
equilibrium (LTE) for the population of atomic levels./TMAP/ is based on
the so-called Accelerated Lambda Iteration (ALI) method and is able to
account for line blanketing by metals. All elements from hydrogen to nickel
may be included in the calculation with model atoms which are tailored for
the aims of the user.http://astro.uni-tuebingen.de/~TMAW/ArchiveSimulationrelated-toTheoSSA When publishing research making use of this service, please
acknowledge: "The TheoSSA service (http://dc.g-vo.org/theossa) used to
retrieve theoretical spectra for this paper was constructed as part of
the activities of the German Astrophysical Virtual Observatory."http://astro.uni-tuebingen.de/~TMAW