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Re: V551 Sgr: drefinite superoutburst of a new SU UMa star! Dear Colleagues, I can see some signature of possible "early superhumps" in Monard's September 21 data (the object was probably experiencing the early relatively rapid fading stage). This is not surprizing, as a long-period system RZ Leo (Psh = 0.078529 d: Ishioka et al. 2001, PASJ 53, 905) also showed the presence of early superhumps, which are the signature of WZ Sge-type dwarf novae (cf. Kato 2002, PASJ 54, L11). The true identification will be made when the exact superhump period is identified. Regards, Taichi Kato VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
