[vsnet-outburst 10087] OT J175130.2+352123: SU UMa-type dwarf nova woth a long superhump period

[Taichi Kato]

OT J175130.2+352123: SU UMa-type dwarf nova woth a long superhump period

   Bart Staels and Kyoto team (observer: Ohshima-san) have reported
observations.  Staels' observations on March 7 showed variations
(~0.3 mag), but the observing window was too narrow to confirm the
periodicity.  Kyoto observation on March 11 showed modulations
(~0.13 mag).  Although it is still difficult to determine the period,
the observations suggests a superhump period of ~2.0 hours.
Further observations are encouraged.