The nature of the recurrent novae

Details The nature of the recurrent novae The nature of the recurrent novae

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...314..653w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 314, March 15, 1987, p. 653-672.

Physics

147

Binary Stars, Novae, Stellar Physics, Main Sequence Stars, Nuclear Fusion, Red Giant Stars, Stellar Mass Accretion, Symbiotic Stars

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

The nature of the recurrent novae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The nature of the recurrent novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The nature of the recurrent novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1452902