Speaker
Description
In this study, we present preliminary stellar parameters of HD 60935 using the spectroscopic and photometric data. We obtained medium resolution spectroscopic data using the Shelyak spectrograph attached to the $0.4$-meter telescope at Ankara University Kreiken Observatory. We utilized two methods to derive stellar parameters: the Bayesian Spectral Energy Distribution Model fitting for photometric data and stellar atmosphere models approaches for spectroscopic data. Stellar atmosphere parameters were derived using equivalent-width measurement and spectral synthesis methods. We also plotted the star on the H-R diagram and estimate its mass, age, radii, metallicity. Our result indicate that HD 60935 is a late type super-giant star with an age of around $0.8$ billion years.
