Identifying blue large amplitude pulsators from Gaia DR2 and ZTF DR3
Blue large amplitude pulsators (BLAPs) are hot, subluminous stars undergoing rapid variability with periods of under 60 min. They have been linked with the early stages of pre-white dwarfs and hot subdwarfs. They are a rare class of variable star due to their evolutionary history within interacting binary systems and the short time-scales relative
McWhirter, Paul Ross et al.
Fecha de publicación:
4
2022