The nature of the recurrent novae

Abstract

view Abstract Citations (185) References (179) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Nature of the Recurrent Novae Webbink, Ronald F. ; Livio, Mario ; Truran, James W. ; Orio, Marina Abstract The basic properties of individual recurrent nova systems are reviewed, and the mechanisms of their outbursts are studied. Some general properties associated with accretion events and thermonuclear runaway models are briefly examined, and detailed models for the recurrent novae T CrB, RS Oph, T Pyx, U Sco, and V1017 Sgr and the possible recurrent novae WZ Sge, V616 Mon, VY Aqr, RZ Leo, V1195 Oph, and V529 Ori are discussed. The results suggest that the outbursts of U Sco and T Pyx are caused by thermonuclear runaways on the surface of massive white dwarfs, while the outbursts of T CrB and RS Oph are very probably accretion events, initiated by a burst of mass transferred from a giant companion onto a main sequence star. V1017 Sgr fails the model criteria for a recurrent nova, being more properly considered a symbiotic star. V1195 Oph, RZ Leo, VY Aqr, and WZ Sge are assigned to the class of dwarf novae. No evidence is found that V529 Ori has recurred. Publication: The Astrophysical Journal Pub Date: March 1987 DOI: 10.1086/165095 Bibcode: 1987ApJ...314..653W Keywords: Binary Stars; Novae; Stellar Physics; Main Sequence Stars; Nuclear Fusion; Red Giant Stars; Stellar Mass Accretion; Symbiotic Stars; Astrophysics; NUCLEOSYNTHESIS; STARS: BINARIES; STARS: NOVAE full text sources ADS | data products SIMBAD (12)