TMAWivo://org.gavo.dc/theossa/q/tmawThe GAVO DC teamRauch, T.2026-01-20T07:42:29ZThomas 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.2018MNRAS.475.3896Rhttp://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/~TMAWhttp://dc.g-vo.org/theossa/q/tmaw/capabilitieshttps://dc.g-vo.org/theossa/q/tmaw/capabilitiesOpticalUV