Re: WZ Sge: superhumps likely evolving Dear Gianluca and Colleagues, > If I remember well, the orbital period is about 82 minutes, > while the period you reported here is around 80 minutes. I > assumed we were waiting for a period longer than Porb to > argue the developing of true superhumps (Patterson et al, > for the 1978 outburst, reported indeed a period 0.8% longer > than Porb). Oh, thanks for the comment. The "nominal" period (as inferred from the period analysis) is now shorter than the orbital period. This may be called as "negative superhumps", but my interpretation is that the true superhump signal is rising at a smaller phase than in early superhumps. The net effect seems to be observed as a "shortening of the mean period". I will make a more detailed analysis, using a longer baseline observations later. Regards, Taichi Kato VSNET Collaboration team