Accretion-disc radius variations in close binaries

Details Accretion-disc radius variations in close binaries Accretion-disc radius variations in close binaries

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.2857h&link_type=abstract

Advances in Space Research, Volume 38, Issue 12, p. 2857-2861.

Physics

1

Scientific paper

Outer radius variations play an important role in the disc structure and evolution. We consider theoretical and observational consequences of such variations in cataclysmic binaries and low-mass X-ray binaries. We find that the action of tidal torques must be important well inside the tidal radius. We also conclude that it is doubtful that the tidal thermal instability is responsible for the superoutburst/superhump phenomena.

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