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[vsnet-outburst 3238] V632 Cyg outburst photometry
V632 Cyg outburst photometry
Dear Colleagues,
We have finished analyzing the Kyoto Dec. 12 observation. The data seem
to show slow modulations (amplitude ~0.1 mag) with a time-scale of ~2 hr.
The periodicity has not been confirmed because of the temporary intereference
by clouds. This modulation could be a hint of emerging superhumps; since
the present outburst is a long, bright one rarely seen in recent years,
further intensive observations are strongly encouraged.
Astrometric identification of the quiescent counterpart is in progress
by Yamaoka-san.
Regards,
Taichi Kato
VSNET Collaboration team
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp