(1992 May 2) subject: further observation of HV Vir Dear Patrick, I could obtain further superhump maxima of HV Vir by CCD photometry at Ouda. May 1.468, 1.530, 1.592 UT. The variable had mean V magnitude of 13.6 (comparison with GSC V=14.4 star). It became fully cloudy and no observations were made for GW Lib. Regards, Taichi Kato
vsnet-adm@kusastro.kyoto-u.ac.jp