Stellar evolution from Pulsations: Hot Subdwarf Stars
My research focuses on observational studies of pulsating hot subdwarf stars with the aim of providing the basis for their asteroseismic analysis. The physical parameters derived by asteroseismology are then used to discriminate between different evolutionary models which is the utmost goal of this research..
Professor: Maja Vuckovic
Image: Pulsating stars across HR diagram, by Prof. J. Christensen-Dalsgaard