Observational asteroseismology of hot subdwarf stars
Observational asteroseismology of hot subdwarf stars
Abstract Hot subdwarf stars are particularly challenging for asteroseismology due to their rapid pulsation periods, intrinsic faintness and relative rarity both in the field and in clusters. These features have ensured that the preferred method of observation up to now has been white‐light photometry, and all asteroseismological solutions to date …