SS Cygni

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stars, Individual Stellar Objects

Scientific paper

SS Cygni (SS Cyg) is a long orbital period (Porb=6.6 h) cataclysmic
variable of the dwarf nova (DN) subclass, characterized by semiperiodic
brightness changes due to outbursts. This CLOSE BINARY STAR consists of
a WHITE DWARF primary which accretes matter from a low-mass,
ROCHE-LOBE-filling secondary star....

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