Detection of a 0.1802-day periodic signal in TESS photometry of slow-rising nova PGIR22akgylf interpreted as orbital modulation from binary distortion of the envelope during common-envelope interaction.
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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.
citing papers explorer
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TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf
Detection of a 0.1802-day periodic signal in TESS photometry of slow-rising nova PGIR22akgylf interpreted as orbital modulation from binary distortion of the envelope during common-envelope interaction.
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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.