Activity of the dwarf nova CH UMa

Details Activity of the dwarf nova CH UMa Activity of the dwarf nova CH UMa

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..947s&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Other

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Cataclysmic Binaries, Symbiotic Stars, X-Ray Sources, X-Ray Bursts

Scientific paper

The outbursts in CH UMa can be divided into two classes (bright and faint), the division magnitude being 12 magvis and separation almost 2 magvis. The maximum brightness of the outbursts tends to decrease over 25 years. The bright outbursts fall into two subtypes according to their decay branches. The recurrence time of the bright outbursts 300-370 days displays variations with a strong secular trend. .

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