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V982 Oph: possible superhumps? Dear Colleagues, Based on the analysis of Torii-san's March 11 data, we have confirmed the object's identity using PSF fitting. The light curve seems to suggest the presence of ~0.2 mag variation, which look like superhumps with a period of ~0.075 d. There was no rapidly fading trend. Owing to the short visibility and the faintness of the object, the identification of this period is not yet clear. With the coming new data sets, we hope we will be able to draw a more definite conclusion. Further observation are encouraged. Regards, Taichi Kato VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
