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dwarf novae

   Also found in: Wikipedia 0.01 sec.
dwarf novae [¦dwȯrf ′nō‚vī]
(astronomy)
A class of irregular variable stars which undergo rapid increases in brightness of several magnitudes at semiperiodic intervals, and then decrease more slowly to the normal minimum; they may be divided into U Geminorum stars and Z Camelopardalis stars.


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Introduction Dwarf novae are a class of cataclysmic variable (CV) star in which a white dwarf primary accretes material from a secondary star via Roche lobe overflow.
Most dwarf novae reach maximum light in a few hours, however both outbursts of V630 Cas were slow affairs.
Introduction Dwarf novae are a class of cataclysmic variable star in which a white dwarf primary accretes material from a secondary star via Roche lobe overflow.
 
 
 
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