Detection of a micronova burst in TESS data of IGR J17014-4306, with inferred burned mass 1.6e-11 solar masses and recurrence time ~20 days, adding the eighth confirmed system.
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Statistical analysis of T CrB light curves finds no robust orbital-phase locking for active phases or eruptions.
citing papers explorer
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A micronova burst in the intermediate polar IGR J17014-4306
Detection of a micronova burst in TESS data of IGR J17014-4306, with inferred burned mass 1.6e-11 solar masses and recurrence time ~20 days, adding the eighth confirmed system.
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Lack of Significant Orbital-Phase Locking in the Active Phases of the Recurrent Nova T CrB
Statistical analysis of T CrB light curves finds no robust orbital-phase locking for active phases or eruptions.