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The SW Sextantis stars

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arxiv astro-ph/9906089 v1 pith:XOILJBL7 submitted 1999-06-04 astro-ph

Coel Hellier (Keele University) This is my paper · ORCID
classification astro-ph
keywords accretiondiscstarsbalancedbehaviourcausedcombinedepisodes
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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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Cited by 1 Pith paper

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  1. Fast optical spectroscopic observations of PSR J1023+0038 over one orbital period

    astro-ph.HE 2026-07 accept novelty 6.0 of 10

    Full-orbit minute-cadence optical spectroscopy of PSR J1023+0038 reveals short-timescale line variability and asymmetric Doppler maps consistent with outflows.

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