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Spectral synthesis of CARMENES M-type stars: stellar atmospheric parameters

MPS-Authors

Lázaro,  F. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Montes,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tabernero,  H. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Marfil,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Caballero,  J. A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

González Hernández,  J. I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Consortium,  CARMENES
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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引用

Lázaro, F. J., Montes, D., Tabernero, H. M., Marfil, E., Caballero, J. A., González Hernández, J. I., & Consortium, C. (2019). Spectral synthesis of CARMENES M-type stars: stellar atmospheric parameters.


引用: https://hdl.handle.net/21.11116/0000-0005-D331-5
要旨
We show our very first results regarding the stellar atmospheric parameter determinations (T_{eff} , log g, [Fe/H]) of M-type stars observed with CARMENES te{Carmenes} by means of the spectral synthesis method. We have selected spectral ranges around iron and titanium lines and molecular bands in three reference M-type stars: GX And (M1.0 V), Luyten's star (M3.5 V),and Teegarden's star (M7.0 V). We employ PHOENIX stellar model atmospheres te{Phoenix}, the radiative transfer code TurboSpectrum te{TurboSpectrum} and line data from the VALD3 database te{Vald} to obtain a grid of synthetic spectra, and a Markov Chain Monte Carlo process implemented in SteParSyn code te{SteParSyn} to derive the value of the stellar atmospheric parameters.