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[vsnet-alert 5708] CP Dra photometry preliminary result



CP Dra photometry preliminary result

   Preliminary analysis of a part of the Kyoto CP Dra run (0.06 d long)
shows no apparent variations greater than 0.1 mag.  There are natural
possibilities that superhumps have not developed yet, or the object may
be an another large-amplitude V344 Ori-like star, or something else (?)

   Only further observations can discriminate the possibilities!  Please
go as long as possible!

Regards,
VSNET Collaboration team

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