TESS data yield a fast white-dwarf spin-down rate in V1405 Cas indicating a propeller regime, a previously unknown 1.36-day orbital period in V1716 Sco, and confirmed periods in V1674 Her, highlighting unexpected properties of accreting white dwarfs.
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A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her
TESS data yield a fast white-dwarf spin-down rate in V1405 Cas indicating a propeller regime, a previously unknown 1.36-day orbital period in V1716 Sco, and confirmed periods in V1674 Her, highlighting unexpected properties of accreting white dwarfs.