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[vsnet-alert 6192] WZ Sge: true superhumps there?



Dear Colleagues,
for what is worth, I would like to point your attention to a quite interesting result.

As I said, my latest photometry (a 6.5 hours long) gives, if considered alone, a period
candidate of 0.057299d. Compared with the shorter, orbital period (0.05669d), I have a
difference of about 1 percent, not so different from what reported by Patterson et al.
during the 1978 outburst (0.8 percent). Just a coincidence? Time will says us!

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         *
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