The recurrent nova U Scorpii revisited - Can a certain class of models be eliminated?

Details The recurrent nova U Scorpii revisited - Can a certain class of models be eliminated? The recurrent nova U Scorpii revisited - Can a certain class of models be eliminated?

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...360..232d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 360, Sept. 1, 1990, p. 232-238. Research supported by Technion - Israel Ins

Physics

7

Novae, Stellar Models, Stellar Physics, Magnetohydrodynamic Stability, Scorpius Constellation, Stellar Envelopes, White Dwarf Stars

Scientific paper

Theoretical models for the recurrent nova U Sco are identified and discussed. In particular, the possible relevance of disk instability models are examined when account is taken of the helium-rich character of the material observed in the disk in quiescence. Even with the assumption of a pure helium disk, it is concluded that it is extremely unlikely that the outbursts of U Sco (and the very similar recurrent nova V394 CrA) are attributable to a disk instability.

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