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

Bibcode
2019hsax.conf..416L
Lázaro, F. J.; Montes, G.; Tabernero, H. M.; Marfil, E.; Caballero, J. A.; González Hernández, J. I.; CARMENES Consortium
Referencia bibliográfica

Highlights on Spanish Astrophysics X, Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain, ISBN 978-84-09-09331-1. B. Montesinos, A. Asensio Ramos, F. Buitrago, R. Schödel, E. Villaver, S. Pérez-Hoyos, I. Ordóñez-Etxeberria (eds.) p. 416-417

Fecha de publicación:
3
2019
Número de autores
7
Número de autores del IAC
2
Número de citas
1
Número de citas referidas
1
Descripción
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.
Tipo
Sin árbitro

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