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[vsnet-obs 26424] RE: [vsnet-alert 4244] SW UMa: superhump evolved
- Date: Fri, 18 Feb 2000 22:02:09 +0100 (MET)
- To: Makoto Uemura <uemura@kusastro.kyoto-u.ac.jp>, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Jochen.Pietz@t-online.de (Jochen Pietz)
- Subject: [vsnet-obs 26424] RE: [vsnet-alert 4244] SW UMa: superhump evolved
- In-Reply-To: <200002181532.AAA23479@pallas.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
On 18-Feb-00 Makoto Uemura wrote:
>
>SW UMa: superhump evolved
>
> In the light curve of SW UMa on Feb. 16 observed at Kyoto,
>we see the evolution of the superhump whose amplitude varied
>from about 0.1 mag to 0.2 mag within 10 hours. The following
>observation by B. Martin showed the 7 superhumps with almost
>constant amplitude of 0.2 mag. The observations are urged
>to catch the more evolutional scenario of superhump.
>
>Regards,
>Makoto Uemura, Taichi Kato and Brian Martin
>
Below you found the links to my lightcurves (through clouds)
2000-02-13.78 to 13.92 (no prominent hump) mean ~10.8mag
http://home.t-online.de/home/Jochen.Pietz/swuma01.gif
2000-02-16.77 to 13.89 (hump with 0.15mag) mean ~11.1mag
http://home.t-online.de/home/Jochen.Pietz/swuma02.gif
2000-02-17.78 to 13.90 (hump with 0.35mag) mean ~11.2mag
http://home.t-online.de/home/Jochen.Pietz/swuma03.gif
Regards,
Jochen Pietz
Return to Daisaku Nogami
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