REVIEW 1 cited by
The SW Sextantis stars
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
The SW Sextantis stars
read the original abstract
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.
Forward citations
Cited by 1 Pith paper
-
Fast optical spectroscopic observations of PSR J1023+0038 over one orbital period
Full-orbit minute-cadence optical spectroscopy of PSR J1023+0038 reveals short-timescale line variability and asymmetric Doppler maps consistent with outflows.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.