VY Scl CV low states

Details VY Scl CV low states VY Scl CV low states

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20515903k&link_type=abstract

American Astronomical Society Meeting 205, #159.03; Bulletin of the American Astronomical Society, Vol. 36, p.1611

Astronomy and Astrophysics

Astronomy

Scientific paper

Fourteen years of photometric CV monitoring has provided a unique data set on ˜ 65 nova-like and 8 magnetic systems, a small fraction of which display large (2-5 mag) drops in their optical light curves (VY Scl states). The speeds and shapes of the transitions for magnetic (polar) and non-magnetic systems are discussed. The character of the transitions in the disk-type VY Scl system appear to be consistent with disruption of mass transfer due to starspots migrating under the L1 point. The transitions in polars, varying from system to system, are difficult to fit into the same picture.

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