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[vsnet-campaign 331] re QW Ser congratulations!
> These results lead to a supercycle of 277 d, which is typical for an SU UMa
> star of this superhump period.
The dates for Takamizawa's 12.8p detections logged in:
http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/obs11000/msg00016.html
are interesting in this light.
[if possible intervening events can be considered as missed].
Cheers
John
vsnet-adm@kusastro.kyoto-u.ac.jp
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