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V877 Ara refined superhump period Dear Colleagues, We have received new data from Roland Santallo. The object still show vigorous superhumps. The best superhump period determined from the 2.2-d baseline is 0.08450(5) d. This period confirms that V877 Ara belongs to a member of long-period SU UMa-type dwarf novae. As in the case of V359 Cen, further obseravations (esp. superhump timing observations) are still highly wanted. Regards, Taichi Kato on behalf of the VSNET Collaboration team
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
