The Tübingen NLTE Model-Atmosphere Package (TMAP) 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 metal-line blanketing. All elements from hydrogen to Barium may be included in the calculation with model atoms which are individually tailored for the aims of the user.
For a more detailed description, see Werner & Dreizler 1999, Werner at al. 2003,TMAP Rauch & Deetjen 2003, or the User's Guide (below).
For the creation of plots, we recommend the use of WRPLOT
Registered users of TMAP can order the most recent version of TMAP!
Solar abundances used by TMAP
Please do not hesitate to contact us in case of any question.
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