Spectral synthesis of CARMENES M-type stars: stellar atmospheric parameters
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)
Lázaro, F. J. et al.
Advertised on:
3
2019