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Title:
A PHOENIX Model Atmosphere Grid for Gaia
Authors:
Brott, I.; Hauschildt, P. H.
Publication:
Proceedings of the Gaia Symposium "The Three-Dimensional Universe with Gaia" (ESA SP-576). Held at the Observatoire de Paris-Meudon, 4-7 October 2004. Editors: C. Turon, K.S. O'Flaherty, M.A.C. Perryman. From http://www.rssd.esa.int/index.php?project=Gaia&page=Gaia_2004_Proceedings, supercedes printed version, p.565
Publication Date:
01/2005
Origin:
ADS
Keywords:
Stars atmospheres, Stars late-type, Radiative transfer, Gaia
Bibliographic Code:
2005ESASP.576..565B

Abstract

We present the results of a set of model atmospheres and synthetic spectra computed with the PHOENIX code. The models cover a range of effective temperatures (2 700 K ≤ Teff ≤ 10 000 K), gravities (‑0.5 ≤ log(g) ≤ 5.5) and metallicities (‑4.0 ≤ [Z/H] ≤ +0.5). In addition, variations of alpha elements are considered for each metallicity. The models are computed with a homogeneous set of input data in order to allow for direct relative comparison between the models. For example, all models use a mixing length of l/Hp = 2.0. We provide synthetic spectra with a resolution of 0.2 nm from the UV to the infrared for all models. We give a brief overview of the input physics and show illustrative results. All synthetic spectra are available via ftp.

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