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EU CMa: possible superhumps Dear Colleagues, We have partly analyzed the Kyoto data of EU CMa. Although the analysis is very preliminary, there seems to be a suggestion of 0.3-mag variations, which can be attributed to superhumps. If these variations are indeed superhumps, the period looks like to be short (around 0.06 d?), the exact identification pending further analysis and observation. The images have been relayed to Yamaoka-san for accurate astrometry and quiescent identification. Depending on the outburst amplitude, the object even may be a WZ Sge-type candidate. The object looks like to be a promising target. We encourage further detailed time-series photometry! Regards, Taichi Kato VSNET Collaboration team
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