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A grid of MARCS model atmospheres for late-type stars

Astronomy and Astrophysics · 2008 · Vol. 486(3) · pp. 951–970
B. GustafssonB. EdvardssonKimmo ErikssonU. G. JørgensenÅke NordlundB. Plez

Abstract

Context. In analyses of stellar spectra and colours, and for the analysis of integrated light from galaxies, a homogeneous grid of model atmospheres of late-type stars and corresponding flux spectra is needed.

Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchAstrophysics and Star Formation StudiesStarsAstrophysicsPhysicsHomogeneousContext (archaeology)Spectral lineFlux (metallurgy)Stellar atmosphereAstronomyMaterials science

Funding

  • Centre National de la Recherche Scientifique
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References
Model atmospheres for G, F, A, B, and O stars
The Astrophysical Journal Supplement Series · 1979 · 1,959 citations
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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