CP Dra
J. Pietz detected an outburst (15.3mag) of this long-period SU UMa-type
dwarf nova on March 27. He also detected a superhump with an amplitude
of 0.2-0.25mag on March 28. The Kyoto team confirmed the outburst and
an evolved superhump with an amplitude of 0.4mag on March 31. The last
superoutburst occurred in 2001 February (vsnet-campaign-dn
2213, 2216,
2214).
M. Uemura reported that the light curve taken at Kyoto on March 31
showed humps with a period of about 0.064 d. This is quite shorter than
that previously reported (0.08348 d). (vsnet-campaign-dn
2236). The object faded from the outburst on April 4 (vsnet-campaign-dn
2271).