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SW UMa post-superoutburst behavior Dear Colleagues, We have finished analyzing the Nov. 16 data from Tanabe-san (VSNET Okayama Station). We have also finished anlyzing the Kyoto Nov. 17 data. On Nov. 16, SW UMa seems to have become slightly brighter than on the previous nights, breaking the slow declining trend. Short-term variations with time-scales of 10-20 min are strongly present. Some of them seem to show some degree of conherence. Some of the variations look like to be associated with late superhumps and their harmonics. From these observation, SW UMa is confirmed to remain active. Regards, Taichi Kato VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
