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The Recurrent Novae and Their Relation with Classical Novae

AIP Conference Proceedings, 2002
Recurrent novae (RNe) are a subclass of cataclysmic variables classified based on recorded observations of more than one nova outburst. They form a small, but heterogeneous group of objects, with 10 known members, that undergo classical nova‐like outbursts, with the significant differences being in the amplitude and the frequency of the outbursts.
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Studies of Classical and Recurrent Novae

Publications of the Astronomical Society of the Pacific, 1992
Novae belong to the cataclysmic-variable class of objects. These objects are interacting binary star systems consisting of a Roche-lobe filling secondary, on or near the main sequence, losing hydrogen-rich material through the inner-Lagrangian point onto an accretion disk that surrounds the primary, which, in most cases, is a white dwarf.
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The Evolutionary Significance of Recurrent Novae

International Astronomical Union Colloquium, 1979
Within the past few years, it has become increasingly apparent that common novae and dwarf novae must owe their origin to binary systems of much larger initial separation than they now have (Paczynski 1976; Ritter 1975, 1976; Webbink 1975). This was demanded by the realization that the white dwarfs in these binaries are generally quite massive (see for
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New Insights into Classical Novae

Annual Review of Astronomy and Astrophysics, 2021
Laura Chomiuk   +2 more
exaly  

Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool

New Astronomy Reviews, 2021
Jordi Isern   +2 more
exaly  

Recurrent novae

Astrophysics and Space Science, 1995
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Observations of galactic and extragalactic novae

Astronomy and Astrophysics Review, 2020
Massimo Della Valle, Luca Izzo
exaly  

Population synthesis of accreting white dwarfs: rates and evolutionary pathways of H and He novae

Monthly Notices of the Royal Astronomical Society, 2021
Alexander Kemp   +2 more
exaly  

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