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Re: V551 Sgr: drefinite superoutburst of a new SU UMa star! Dear Colleagues, > The superhump period is still rather uncertain (around 0.06 d), but will > be readily refined when the baseline coverage is improved. The best period is probably somewhere around 0.065 d. The system is less likely a very short-period system (as originally inferred from the supposed WZ Sge-type classification), though the appearance of superhumps looks slightly slower than in other SU UMa-type stars. Regards, Taichi Kato VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
