RXJ0640-24 outburst update Dear Colleagues, As notified by Uemura-san, RX J0640-24 is apparently quickly fading from outburst. The possible superhump-like feature observed in the Jan. 7 data seems to have decayed on Jan. 8 data. However, there looks like some evidence of modulations with a likely period less than an hour. During the 3.4-hour run, the object showed little trend of the continuing rapid fading. This precludes the possible explanation of the Jan. 7 variation as the effect of extinction. The rapid rate of decline (~1 mag/day between Jan. 6 and 8) suggests that the object can be a short-period system (e.g. SU UMa stars). It is not surprizing such a system may show transient superhump activities during a short outburst, or a precursor to a superoutburst (the good example is the superoutburst of SU UMa in 1998 December). Observers are strongly requested to continue monitoring the activity of the object for short-term variations on coming nights, and to look for a possible (immediate or future) superoutburst. The campaign is still ongoing, and please keep us in touch. Regards, Taichi Kato and Makoto Uemura