The March 1995 superoutburst of the SU Ursae Majoris star AK Cancri: photometry and superhumps.

Details The March 1995 superoutburst of the SU Ursae Majoris star AK Cancri: photometry and superhumps. The March 1995 superoutburst of the SU Ursae Majoris star AK Cancri: photometry and superhumps.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...315..493m&link_type=abstract

Astronomy and Astrophysics, v.315, p.493-498

Astronomy and Astrophysics

Astrophysics

13

Novae, Cataclysmic Variables, Stars: Individual: Ak Cnc

Scientific paper

We present differential photometry of AK Cnc obtained during its March 1995 superoutburst. Superhumps with amplitude of 0.2mag appeared within 4 days after maximum with a period of 0.06749(1)d. This result is used to estimate a likely orbital period of 0.065(2)d and a mass ratio (M_2_/M_1_) of 0.21. Photometric maxima and timings of 26 recorded outbursts imply an average cycle length of 47 days.

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