Outburst activity in magnetic cataclysmic variables BY Cam and QQ Vul

Details Outburst activity in magnetic cataclysmic variables BY Cam and QQ Vul Outburst activity in magnetic cataclysmic variables BY Cam and QQ Vul

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..402h&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 402-405

Astronomy and Astrophysics

Astrophysics

Scientific paper

Flare properties in magnetic cataclysmic variables BY Cam and QQ Vul are determined based on the observations obtained at AZT-11 and the Shain mirror telescope of the Crimean Astrophysical Observatory. The UBVRI AZT-11 photometry demonstrates a wide range of color properties of these events. There are significant differences between the flare amplitudes in BY~Cam and QQ~Vul. The correlation coefficient between the flare amplitude and smoothed brightness variations of QQ~Vul is of about 0.83. Similar dependence for the flares of BY~Cam is not detected. Some values of the cross-correlation ``brightness-polarization" are as large as 0.7. There are no significant differences between the colors of observed flares, as for instance, one could expect for possible ``accretion" and ``red dwarf" flares.

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