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[vsnet-obs 28012] Re: SW Vul, DO Vul, Var66 Cyg, V660 Her, V795 Cyg
- Date: Sat, 3 Jun 2000 21:30:40 +0200
- To: vsnet-obs@kusastro.kyoto-u.ac.jp, vsnet-outburst@kusastro.kyoto-u.ac.jp, Jochen Pietz <Jochen.Pietz@t-online.de>, Patrick Schmeer <extpasc@rz.uni-sb.de>
- From: Patrick Schmeer <p.schmeer@mx.uni-saarland.de>
- Subject: [vsnet-obs 28012] Re: SW Vul, DO Vul, Var66 Cyg, V660 Her, V795 Cyg
- In-Reply-To: <XFMail.000603161211.Jochen.Pietz@t-online.de>; from Jochen.Pietz@t-online.de on Tue, May 30, 2000 at 08:37:37PM +0200
- References: <200005300445.NAA24296@ceres.kusastro.kyoto-u.ac.jp> <XFMail.000603161211.Jochen.Pietz@t-online.de>
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
On Tue, May 30, 2000 at 08:37:37PM +0200, Jochen Pietz wrote:
> VAR66 Cyg 2000-06-02.025 14.39C comp star GSC 3196.1865
In future please use the designation 'V2209 Cyg'.
In IBVS 4673 Sergei Antipin reports a maximum magnitude of mag 15.25 in B.
His mean lightcurve for the long outbursts shows a flat maximum of 9 days
duration. In my opinion this behavior is more typical for SS Cyg-type dwarf
novae. The short outbursts are almost as bright as the long ones, and the
fading rate for the former seems to be rather small for normal UGSU out-
bursts.
Regards,
Patrick
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