OU Vir: new post-superoutburst observations Dear Colleagues, We have received new observations of OU Vir from Nogami-san (Hida observatory), Donn Starkey, Tom Krajci and Kyoto data. We have also analyzed recently arrived observations from Torii-san (RIKEN, very extensive data sets), and Kiyota-san. The post-superoutburst data confirm the slow fading trend reported in detail yesterday. When the late superhumps are superimposed on orbital humps, the hump amplitude looks greatly enhanced, as we saw in WZ Sge 2001. The eclipse are sharp and deep, mostly amounting for 1.0-1.5 mag in depth. Please keep the current very excellent coverage, until the critical time for a rebrightening passes. Regards, Taichi Kato VSNET Collaboraion team
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