[vsnet-alert 15432] GR Ori: superhump period

[Ohshima]

GR Ori: superhump period

 We have received further observations from Maeda-
san, Itoh-san, Seikei High-school team, and William
Stein. As mentioned in the previous mail, the yielded
superhump period is 0.05714 (4) d. This superhump
period implies that this object is a typical WZ Sge-type 
dwarf nova, in the view of locating near the period
minimum.

 Further observations are encouraged!