BC UMa possible outburst Jose Ripero reports that the SU UMa-type dwarf nova BC UMa may be undergoing an outburst. Confirmatory observations are most urgently requested. YYYYMMDD(UT) mag observer 20010408.326 <138 (M. Simonsen) 20010409.819 <153 (T. Kinnunen) 20010409.853 <138 (E. Muyllaert) 20010410.830 <153 (T. Kinnunen) 20010411.867 <142 (E. Muyllaert) 20010411.891 <140 (J. Ripero) 20010413.867 <142 (E. Muyllaert) 20010413.869 <138 (M. Westlund) 20010413.968 <158 (C. P. Jones) 20010414.226 <142 (M. Simonsen) 20010414.885 141 (J. Ripero) The object underwent a superoutburst in 2000 April, which was followed by a post-superoutburst rebrightening. This superoutburst was exceptionally perfectly followed by the VSNET Collaboration team (cf. vsnet-alert 4522, 4523, 4524, 4530, 4532, 4537, 4553, 4556, 4562, 4567, 4577, 4584, 4586, 4591, 4595, 4601, 4613, 4614, 4665, 4666, 4667, 4668, 4669,0 4670, 4671, 4672). The interval since the 2000 superoutburst may suggest that the present outburst (if confirmed) may be a normal outburst, which has never been observed in recent years (most of BC UMa outbursts are superoutburst, just as in SW UMa, or more exceptionally in WZ Sge). Observations during the present outburst (if confirmed) are very strongly encouraged in order to study the nature of rarely met normal outburst in such systems. A similar system SW UMa is known to show "intermediate outbursts", which have brightness and durations between those of bright superoutbursts and normal outbursts. Past observations of SW UMa during such an outburst has shown ununual development of superhumps. Observers of BC UMa should also bear in mind such an unexpected variation could be recorded. The VSNET Collaboration team is happy to receive any data on this object, either in outburst or quiescence. Please make the best science! Regards, VSNET Collaboration team