SN2003aw = helium dwarf nova? According to IAUC No. 8084, "SN2003aw" looks like to be a hydrogen-deficient dwarf nova resembling KL Dra = SN1998di. The duration of the current bright state suggests a superoutburst, if this type classification is correct. Further observations are naturally encouraged! (From vsnet-campaign-sn 565) SN2003aw 20030114.0 <210C PAL SN2003aw 20030206.26 178C PAL SN2003aw 20030210.0 176C PAL SN2003aw 20030219.0 178C PAL # SN 2003aw (9:05:54.79, -05:36:08.6 (J2000.0), almost superimposed on # the nucleus (within 2")) is hosted by also a dim galaxy. Regards, Taichi Kato
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