Identifying and Quantifying Recurrent Novae Masquerading as Classical Novae
Ashley Pagnotta, Bradley E. Schaefer

TL;DR
This study develops criteria to distinguish recurrent novae from classical novae, revealing that about 24-35% of known Galactic novae may actually be recurrent novae, impacting understanding of supernova progenitors.
Contribution
The paper introduces specific observational criteria to identify recurrent novae among classical novae, estimating a significant hidden population of RNe in our galaxy.
Findings
Approximately 24-35% of known Galactic novae are likely RNe.
Identified new strong RN candidates based on spectral and light curve criteria.
Estimated around 100 hidden RNe are masquerading as classical novae.
Abstract
Recurrent novae (RNe) are cataclysmic variables with two or more nova eruptions within a century. Classical novae (CNe) are similar systems with only one such eruption. Many of the so-called 'CNe' are actually RNe for which only one eruption has been discovered. Since RNe are candidate Type Ia supernova progenitors, it is important to know whether there are enough in our galaxy to provide the supernova rate, and therefore to know how many RNe are masquerading as CNe. To quantify this, we collected all available information on the light curves and spectra of a Galactic, time-limited sample of 237 CNe and the 10 known RNe, as well as exhaustive discovery efficiency records. We recognize RNe as having (a) outburst amplitude smaller than 14.5 - 4.5 * log(t_3), (b) orbital period >0.6 days, (c) infrared colors of J-H > 0.7 mag and H-K > 0.1 mag, (d) FWHM of H-alpha > 2000 km/s, (e) high…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Gamma-ray bursts and supernovae · Particle Accelerators and Free-Electron Lasers
