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[vsnet-alert 7273] V589 Her: results of 2002, Apr 05/06 photometry session at CBA Belgium Observatory
- Date: Sat, 6 Apr 2002 11:08:42 +0200
- To: "cba-news" <news@cba.phys.columbia.edu>
- From: "Tonny Vanmunster" <Tonny.Vanmunster@advalvas.be>
- Subject: [vsnet-alert 7273] V589 Her: results of 2002, Apr 05/06 photometry session at CBA Belgium Observatory
- Cc: "vsnet-campaign-dn" <vsnet-campaign-dn@kusastro.kyoto-u.ac.jp>, "vsnet-alert" <vsnet-alert@kusastro.kyoto-u.ac.jp>, "Vsnet-Outburst" <vsnet-outburst@kusastro.kyoto-u.ac.jp>
- Delivered-To: vsnet-alert@kusastro.kyoto-u.ac.jp
- Importance: Normal
- In-Reply-To: <200204060534.OAA20612@kibitaki.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
Dear colleagues,
I have just concluded the analysis of a 3.1 h (unfiltered) CCD photometry
session of V589 Her, obtained on April 05/06, 2002 at CBA Belgium
Observatory. As usual, a 0.35-m f/6.3 telescope and ST-7 CCD were the main
equipment. Weather conditions during the observing session were moderate :
clear skies but heavy winds.
The resulting light curve will be made available on my web site later today
(www.lunarpages.com/cbabelgium). It shows a periodic (?) modulation with a
0.12 mag amplitude, as was also announced by the Kyoto team in a recent
vsnet message. My observing session was too short to firmly conclude on the
nature of the modulation, but it *might* be the signature of a hump, with a
period of approx 0.1 d. I hope to obtain more observations over a longer
time span, in the next nights, to conclude on this. Important to note is
also that my observations did not reveal any eclipse-like dip (as reported
by the Kyoto team), and the hump profile seems to indicate a rather long
orbital period system.
Needless to say this object deserves all possible attention over the next
nights, through a multi-longitude time-series observing effort.
Kind regards,
Tonny Vanmunster
CBA Belgium Observatory
www.lunarpages.com/cbabelgium
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