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SW UMa post-superoutburst, update Dear Colleagues, We have finished analyzing the Nov. 19 data (from Tanabe-san and Kyoto). The object keeps its post-superoutburst magnitude level. A new humps having a superhump-like profile appeared, although the period is different from ordinary superhumps or late superhumps. Further examination of the data is in progress. Further observations are still wanted to completely illustrate the post-superoutburst behavior. Regards, Taichi Kato VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
