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R. Novak has kindly sent us data sets on December 23 and 24 during
the superoutburst. Combined with his data, the data taken at Kyoto
on December 22, 23, 24, 25, and 26 yields the best candidate of the
superhump period of 0.078483 day, which is slightly shorter than the
previous result. The average superhump light curve is a typical one
for that of SU UMa star in superoutburst.
The outburst have already been terminated, but colse monitorings
for possible re-brightening are encouraged.
Regards,
Makoto Uemura
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
