Abstract:Due to low discovery efficiencies, there must be some number of classical novae (CNe) that are in fact recurrent novae (RNe) for which only one eruption has so far been observed. We collect all available information on the light curves, spectra, and quiescent characteristics of a time-limited sample of 237 Galactic CNe and the ten known Galactic RNe, and identify seven characteristics that are indicative of a short recurrence time: (1) outburst amplitude smaller than 14.5 − 4.5 × log(t 3 ), (2) orbital period … Show more
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