Probing stellar evolution with S stars and Gaia
By: Shreeya Shetye,
Universite Libre de Bruxelles, Belgium
About / Description
In the talk, the focus is to explain how high-resolution spectroscopic data of S stars combined with the Gaia Data Release 2(GDR2) parallaxes and with the MARCS model atmospheres for S-type stars were used to derive effective temperatures, surface gravities, and luminosities.
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