CCD photometry of outbursts in GK Per

Details CCD photometry of outbursts in GK Per CCD photometry of outbursts in GK Per

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..939s&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, Photometric, Polarimetric, And Spectroscopic Instrumentation, X-Ray Sources, X-Ray Bursts

Scientific paper

Photometry of the dwarf nova type 1996 outburst of GK Per shows that the color indices are getting bluer during the late rise to the maximum brightness and a strong linear reddening is visible during the decline. The brightness fluctuations (cycles of 0.055-0.070 days and 0.028-0.045 days) were detected during the 1999 outburst. The amplitude of the fluctuations (intensity units) was increasing during the rise to the maximum light. .

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