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Dwarf Novae in the Shortest Orbital Period Regime: I. A New Short Period Dwarf Nova, OT J055717+683226

Makoto Uemura,Akira Arai,Taichi Kato,Hiroyuki Maehara,Daisaku Nogami,Kaori Kubota,Yuuki Moritani,Akira Imada,Toshihiro Omodaka,Shota Oizumi,Takashi Ohsugi,Takuya Yamashita,Koji S. Kawabata,Mizuki Isogai,Osamu Nagae,Mahito Sasada,Hisashi Miyamoto,Takeshi Uehara,Hiroyuki Tanaka,Risako Matsui,Yasushi Fukazawa,Shuji Sato,Masaru Kino

Publications of the Astronomical Society of Japan（2010）

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摘要
We report on the observation of a new dwarf nova (DN), OT J055717+683226 (OT: optical transient), during the period of its first-recorded superoutburst in 2006 December. Our observation shows that this object is an SU UMa-type dwarf nova having a very short superhump period of 76.67$\pm$0.03 min (0.05324$\pm$0.00002 d). The next superoutburst was observed in 2008 March. The recurrence time of supe...
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关键词
accretion, accretion disks,stars: individual (OT J055717+683226),novae, cataclysmic variables
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