Precise surface gravitites of A-type stars from Asteroseismology
δ Sct are one of the most abundant pulsating stars in our Galaxy. In addition, they have moderate to fast rotations and periods of several hours. That makes them the suitable targets for studying the effects of rotation on stellar evolution. In this work, we show how to infer the mean density and the surface gravity of an A-type pulsanting star
García Hernández, A. et al.
Fecha de publicación:
3
2019