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INTEGRAL and Cataclysmic Variables
AIP Conference Proceedings, 2010The results of investigations of cataclysmic variables (CVs) with the ESA INTEGRAL satellite are briefly presented and discussed. It is evident that the satellite serves as an efficient tool to study some of these objects.
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The Structure of Cataclysmic Variables
Annual Review of Astronomy and Astrophysics, 1976The cataclysmic variables are usually divided into the following four classes: novae; recurrent novae; dwarf novae, which are subclassified as U Geminorum stars or Z Camelopardalis stars; and novalike variables. Those observations that bear most directly on the structure of cataclysmic variables at minimum light are reviewed.
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On the Statistics of Cataclysmic Variables
1995We have conducted a X 2 test of the magnetic field distribution of AM Hers in comparison with isolated white dwarfs. If we use bins with field ranges of 10–29MG, 30–99MG, 100–299MG and >300MG, we obtain a X 2 of 10.1 (3 degrees of freedom). This implies a 100 MG is significant, and the period distribution for AM Hers and the other cataclysmic ...
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