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Re: NSV 10934: superoutburst of a new SU UMa-type dwarf nova! Dear Colleagues, We have just posted a phase-averaged superhump light curve of NSV 10934 at http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/NSV10934/nsvsh.gif There is also a summary page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/nsv10934.html A closer examination of Stockdale's suggests the presence of QPOs (possibly super-QPOs). Together with the rather irregular profile of the superhumps, it is most likely that the superhumps were still in their growing phase. We can then expect a further growth of the amplitudes, and possibly a rapid period change. Further observations are most encouraged! Regards, Taichi Kato VSNET Collaboration team
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