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During the last outburst of UV Gem, the Kyoto team performed
time-series observations on February 11, 13, 15, 16, and 17.
Since February 11, the decline rate has become faster with time.
This behavior and the long-range light curve are not typical
for superoutbursts with a plateau phase, but like a long normal one,
although the decline rate between February 11 and 13 (0.17mag/day)
may be consistent with that during the plateau phase.
We have obtained long-runs on February 13 and 15. The light curves
show no prominent periodic modulation with an amplitude over 0.1mag.
Regards,
Makoto Uemura
Return to the Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp
