Dear Colleagues, a look to a subset (1.7 hours) of my last run (July 27/28) on this star is very interesting. The resulting lightcurve clearly says that deep changes are undergoing there. This is a partial result, but it is clear that the structure seen until now is definitely evolved in a more complex lightcurve. Many peaks now appeared, where we had mainly two series of them. The difference in amplitude among them is now smaller. Maybe that normal superhumps are starting to appear, but I need to analyze all the run. But what it is surely true is that something important happened. As always, you cas see lightcurves at http://vsnet.eurolink.it/comets/wzsge.htm Regards, Gianluca -- *********************************************************************** * Gianluca Masi "Two things fill the soul * * Via Madonna de Loco, 47 with awe and reverence [...]: * * 03023 Ceccano (FR) the starry sky above me and * * ITALY the moral law within me" * * e-mail: gianmasi@fr.flashnet.it * * web: http://vsnet.eurolink.it/comets/ I. Kant * * Minor Planet Center Obs. Code: 470 - Ceccano * * Center for Backyard Astrophysics - Italy * * VSNET Collaboration Team member * * CCD-astrometry-photometry@egroup.com mailing-list moderator * ***********************************************************************