M31N 2017-01e is likely a recurrent nova powered by a white dwarf accreting from the decretion disc of a Be star companion, rather than from a late-type star.
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Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?
M31N 2017-01e is likely a recurrent nova powered by a white dwarf accreting from the decretion disc of a Be star companion, rather than from a late-type star.