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On the Frequency of Occurrence of Recurrent Novae and Their Role as Type Ia Supernova Progenitors

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© 1996. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Massimo Della Valle and Mario Livio 1996 ApJ 473 240 DOI 10.1086/178139

0004-637X/473/1/240

Abstract

We have determined the frequency of occurrence of recurrent novae (RNe) for the Galaxy, M31, and the LMC. We find that the ratio between the rate of outbursts of recurrent and classical novae (CNe) is in the range nout(RNe)/nout(CNe) ~ 0.1-0.3. The implications of this result for the realization frequency of RNe as potential progenitors of Type Ia supernovae are also discussed. RNe are not the major class of progenitors of Type Ia supernovae.

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10.1086/178139