Evolved compact pulsators found primarily amongst the white dwarf and hot subdwarf populations provide important seismic windows over the late stages of stellar evolution of low-to-intermediate mass stars, past the red-giant branch. These windows are particularly welcomed as uncertainties in modeling the core helium-burning phase and beyond are still prominent and pile-up, impacting strongly...
75. Testing models of ultimate stages of stellar evolution with asteroseismology of evolved compact pulsators: achievements and prospects in the Gaia era (Invited)
9/22/22, 4:30 PM