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Aims. We present a new library of high-resolution synthetic spectra based on the stellar atmosphere code PHOENIX that can be used for a wide range of applications of spectral analysis and stellar parameter synthesis.
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Tim-Oliver Husser
S. Berg
S. Dreizler
Astronomy and Astrophysics
Centre National de la Recherche Scientifique
Universität Hamburg
Université Claude Bernard Lyon 1
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Husser et al. (Sat,) studied this question.
www.synapsesocial.com/papers/69d809c605ee2ba81dbeec3b — DOI: https://doi.org/10.1051/0004-6361/201219058