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[vsnet-alert 6192] WZ Sge: true superhumps there?
- Date: Sat, 04 Aug 2001 08:03:23 +0200
- To: VSNET ALERT <vsnet-alert@kusastro.kyoto-u.ac.jp>, vsnet-campaign-dn <vsnet-campaign-dn@kusastro.kyoto-u.ac.jp>, cba-news <news@cba.phys.columbia.edu>
- From: Gianluca Masi <gianmasi@fr.flashnet.it>
- Subject: [vsnet-alert 6192] WZ Sge: true superhumps there?
- Organization: "Bellatrix" Astronomical Observatory
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
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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