Following the initial alert by Michael Mattiazzo (vsnet-alert 802), following observations have been reported to vsnet-alert and vsnet-obs. YYMMDD(UT) mag code 970312.497 <127 MKA 970316.433 <127 MKA 970325.424 117 MKA 970325.453 116 MKA 970325.562 116 MKA 970326.417 114 MKA 970326.458 115 MKA 970326.500 116 MKA 970326.542 115 MKA 970326.801 111 HJN Judging from the brightness and duration, the present outburst may well be a superoutburst, since its last one in 1995 October - November. OY Car is one of the most well-known eclipsing SU UMa-type dwarf novae, which have been and will be teaching us much about the physical processes going in superoutbursting dwarf novae. OY Car has played an important role in this field [1,2,3]. [1] J. H. Wood et al., 1989, ApJ 341, 974 [2] F. V. Hessman et al., 1992, AsAp 263, 147 (OY Carinae: the secrets of the super-humps revealed) [3] I. Billington et al., 1996, MNRAS, 279, 1274 and references therein I would also like to urge visual (and CCD, of course) observers to record spectacular eclipses (together with possible superhumps) of this short-period cataclysmic binary. A good northern example may be found at (http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/htcas.html). According to [1], eclipse are expected to occur: HJED = 2443993.553691 + 0.0631209295 E +/-50 +/-20 Regards, Taichi Kato