Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-06-04
Astronomy and Astrophysics
Astrophysics
To appear in proc. Warner Symposium on Cataclysmic Variables
Scientific paper
10.1016/S1387-6473(00)00026-9
I review the observational properties of SW Sex stars. I show that they can
be explained by an accretion stream overflowing the disc, combined with an
accretion disc wind. I suggest that SW Sex behaviour is caused by episodes of
very high mass transfer, which are balanced by VY Scl low states.
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