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PU CMa: post-superoutburst fading Dear Colleagues, We have received a new data set from Berto Monard. PU CMa is slowly fading (post-superoutburst stage). Late superhumps are very prominent throughout this post-superoutburst stage. We have also received a successful report of observation from Peter Nelson. We will make a further analysis after receiving this full report. The long persistence of late superhumps is one of the signatures of short-period SU UMa stars. These stars frequently undergo post-superoutburst rebrighteng(s) -- so please watch carefully!! Regards, Taichi Kato VSNET Collaboration team
Return to the Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
