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Start Over Subject stellar-atmospheres Publisher The GAVO DC team Resource Type Simulation
1. PoWR
ID:
ivo://org.gavo.dc/gvo/data/PoWR/powr.ipap
Title:
PoWR
Short Name:
PoWR
Date:
23 Mar 2022 13:13:05
Publisher:
The GAVO DC team
Description:
Theoretical spectral energy distributions (SEDs) from expanding NLTE model atmospheres for hot stars.
2. TheoSSA - Theoretical Stellar Spectra Access
ID:
ivo://org.gavo.dc/theossa/q/ssa
Title:
TheoSSA - Theoretical Stellar Spectra Access
Short Name:
theossa
Date:
23 Mar 2022 13:13:07
Publisher:
The GAVO DC team
Description:
TheoSSA provides spectral energy distributions based on model atmosphere calculations. Currently, we serve results obtained using the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact stars.
3. TheoSSA TMAP Web Interface
ID:
ivo://org.gavo.dc/theossa/q/web
Title:
TheoSSA TMAP Web Interface
Short Name:
tmap_web
Date:
23 Mar 2022 13:13:07
Publisher:
The GAVO DC team
Description:
TheoSSA provides spectral energy distributions based on model atmosphere calculations. Currently, we serve results obtained using the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact stars.
4. TMAW -- Tübingen Model Atmosphere Package WWW Interface
ID:
ivo://org.gavo.dc/theossa/q/tmaw
Title:
TMAW -- Tübingen Model Atmosphere Package WWW Interface
Short Name:
TMAW
Date:
23 Mar 2022 13:13:07
Publisher:
The GAVO DC team
Description:
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.