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BO Ceti: Dwarf nova showing both IW And-type and SU UMa-Type features

Taichi Kato,Yusuke Tampo,Naoto Kojiguchi,Masaaki Shibata,Junpei Ito,Keisuke Isogai,Hiroshi Itoh,Franz-Josef Hambsch,Berto Monard,Seiichiro Kiyota,Tonny Vanmunster,Aleksei A. Sosnovskij,Elena P. Pavlenko,Pavol A. Dubovsky,Igor Kudzej,Tomas Medulka

Publications of the Astronomical Society of Japan（2021）

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Abstract
IW And stars are a recently recognized subgroup of dwarf novae which are characterized by (often repetitive) slowly rising standstills terminated by brightening, but the exact mechanism for this variation is not yet identified. We have identified BO Cet, which had been considered as a novalike cataclysmic variable, as a new member of IW And stars based on its behavior in 2019–2020. In addition to ...
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accretion, accretion disks,novae, cataclysmic variables,stars: dwarf novae,stars: individual (BO Ceti)
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