The sw sextantis stars - INSPIRE

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The sw sextantis stars

Coel Hellier

Jun, 1999

Published in:

New Astron.Rev. 44 (2000) 131

e-Print:

astro-ph/9906089 [astro-ph]

DOI:

10.1016/S1387-6473(00)00026-9

View in:

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Abstract: (arXiv)

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.

References(34)

Figures(0)

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