A new extensive library of PHOENIX stellar atmospheres and synthetic spectra
Tim-Oliver Husser1, Sebastian Wende – von Berg1, Stefan Dreizler1, Derek Homeier12, Ansgar Reiners1, T. Barman3, and Peter H. Hauschildt4
1Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany
2CRAL, UMR 5574, CNRS, Université de Lyon, École Normale Supérieure de Lyon, 46 Allée d’Italie, F-69364 Lyon Cedex 07, France
3Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ, 86001, USA
4Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany
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.
Methods. The spherical mode of PHOENIX was used to create model atmospheres and to derive detailed synthetic stellar spectra from them. We present a new self-consistent way of describing micro-turbulence for our model atmospheres.
Results. The synthetic spectra cover the wavelength range from 500Å to 5.5μm with resolutions of R = 500 000 in the optical and near IR, R = 100 000 in the IR and λ=0.1Å in the UV. The parameter space covers 2 300 K < Teff < 8 000 K, 0.0 < log(g) < +6.0, -4.0 < [Fe/H] < +1.0 and -0.2 < [α/M] < +1.2. The library is a work in progress and going to be extended to at least Teff = 25 000 K.
Please cite this paper when using spectra from our spectral library!