AO Oct outburst continues Rod Stubbings reports that the rare outburst of AO Oct continues. The fade of 0.8 mag in three days may look rapid for typical superoutbursts of SU UMa stars. This may suggest that AO Oct is an SS Cyg type dwarf nova, or may belong to large-amplitude rapid faders among SU UMa-type systems, like V592 Her. Time-resolved photometry is most urgently wanted! Regards, Taichi Kato VSNET Collaboration team