The Potential of Asteroseismology for Hot, Subdwarf B Stars: A New Class of Pulsating Stars?
The Potential of Asteroseismology for Hot, Subdwarf B Stars: A New Class of Pulsating Stars?
We present key sample results of a systematic survey of the pulsation properties of models of hot B subdwarfs. We use equilibrium structures taken from detailed evolutionary sequences of solar metallicity (Z = 0.02) supplemented by grids of static envelope models of various metallicities (Z = 0.02, 0.04, 0.06, 0.08, …