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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.
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B. Gustafsson
Nordic Institute for Theoretical Physics
B. Edvardsson
Uppsala University
Kimmo Eriksson
University of California, Davis
Astronomy and Astrophysics
Université de Montpellier
Netherlands Institute for Radio Astronomy
Astronomy and Space
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Gustafsson et al. (Thu,) studied this question.
synapsesocial.com/papers/6a078fcbc9983f2ec4c64235 — DOI: https://doi.org/10.1051/0004-6361:200809724