Revision as of 15:06, 24 August 2017 edit Headbomb (talk \| contribs) Edit filter managers, Autopatrolled, Extended confirmed users, Page movers, File movers, New page reviewers, Pending changes reviewers, Rollbackers, Template editors 473,581 edits →Cataclysmic variables: ce ← Previous edit		Revision as of 15:07, 24 August 2017 edit undo Headbomb (talk \| contribs) Edit filter managers, Autopatrolled, Extended confirmed users, Page movers, File movers, New page reviewers, Pending changes reviewers, Rollbackers, Template editors 473,581 edits →Cataclysmic variables: Publ. Astron. Soc. Pac. Next edit →
Line 35: Apparently the only SSXS nonmagnetic cataclysmic variable is V Sge: bolometric luminosity of (1 - 10) x 10<sup>37</sup>, a binary including a blackbody (BB) accretor at T < 80 eV, and an orbital period of 0.514195 d.<ref name=Greiner/> The accretion disk can become thermally stable in systems with high mass-transfer rates (Ṁ).<ref name=Kato/> Such systems are called nova-like (NL) stars, because they lack outbursts characteristic of dwarf novae.<ref name=Osaki>{{ cite journal \|doi=10.1086/133689 \|last1=Osaki \|first1=Yoji \|title=Dwarf-Nova Outbursts \|journal=~~PASP~~Publ. Astron. Soc. Pac. \|date=1996 \|volume=108 \|pages=39 \|bibcode=1996PASP..108...39O }}</ref> ==VY Scl cataclysmic variables==

Supersoft X-ray source: Difference between revisions