Cataclysmic variable star
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Cataclysmic variable stars (CV) are stars which irregularly increase in brightness by a large factor, then drop back down to a quiescent state. They were initially called novae, from the Latin 'new', since ones with an outburst brightness visible to the naked eye and a quiescent brightness invisible appeared as new stars in the sky.
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The Catalog and Atlas of Cataclysmic Variables The Catalog and Atlas of Cataclysmic Variables archive.stsci.edu/prepds/cvcat/index.html - Web |
TPP/CVcat - a catalogue of Cataclysmic Variable St... TPP/CVcat - a catalogue of Cataclysmic Variable Stars www.cvcat.net - Web |
RKcat (Ritter and Kolb), 7th edition RKcat (Ritter and Kolb), 7th edition www.mpa-garching.mpg.de/RKcat/ - Web |
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CVNet, a web site and community for CV enthusiasts... CVNet, a web site and community for CV enthusiasts and researchers sites.google.com/site/aavsocvsection/ - Web |
A Beginner's Guide to Cataclysmic Variables A Beginner's Guide to Cataclysmic Variables www.mssl.ucl.ac.uk/www_astro/gal/cv_beginners.html - Web |
Cataclysmic Variables Cataclysmic Variables heasarc.gsfc.nasa.gov/docs/objects/cvs/cvstext.html - Web |