High-speed photometry of 16 candidate white dwarfs revealed three new pulsating white dwarfs (one ELM, one low-mass, one ZZ Ceti) and three new binary systems with ellipsoidal or reflection variability.
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Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems
High-speed photometry of 16 candidate white dwarfs revealed three new pulsating white dwarfs (one ELM, one low-mass, one ZZ Ceti) and three new binary systems with ellipsoidal or reflection variability.