A grid of MARCS model atmospheres for late-type stars
B. GustafssonDepartment of Physics and Astronomy, Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden e-mail: [Bengt.Gustafsson;bg]@astro.uu.seB. EdvardssonDepartment of Physics and Astronomy, Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden e-mail: [Bengt.Gustafsson;bg]@astro.uu.seKimmo ErikssonDepartment of Physics and Astronomy, Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden e-mail: [Bengt.Gustafsson;bg]@astro.uu.seU. G. JørgensenÅke NordlundB. PlezDepartment of Physics and Astronomy, Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden e-mail: [Bengt.Gustafsson;bg]@astro.uu.se
2008en
ABI
Annotatsiya
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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