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Multi-wavelength Photometry During the 2018 Superoutburst of the WZ Sge-type Dwarf Nova EG Cancri

Mariko Kimura,Keisuke Isogai,Taichi Kato,Naoto Kojiguchi,Yasuyuki Wakamatsu,Ryuhei Ohnishi,Yuki Sugiura,Hanami Matsumoto,Sho Sumiya,Daiki Ito,Kengo Nikai,Katsura Matsumoto,Sergey Yu Shugarov,Natalia Katysheva,Hiroshi Itoh,Pavol A. Dubovsky,Igor Kudzej,Hiroshi Akitaya,Kohei Oide,Takahiro Kanai,Chihiro Ishioka, Yoshinori Uzawa,Yumiko Oasa,Tonny Vanmunster,Arto Oksanen,Tamas Tordai,Katsuhiro L. Murata,Kazuki Shiraishi,Ryo Adachi,Motoki Oeda,Yutaro Tachibana,Seiichiro Kiyota,Elena P. Pavlenko,Kirill Antonyuk,Oksana Antonyuk,Nikolai Pit,Aleksei Sosnovskij,Julia Babina, Alex Baklanov,Koji S. Kawabata,Miho Kawabata,Tatsuya Nakaoka,Masayuki Yamanaka,Kiyoshi Kasai,Ian Miller,Stephen M. Brincat,Wei Liu,Mahito Sasada,Daisaku Nogami

Publications of the Astronomical Society of Japan（2020）

Cited 7|Views51
Key words
accretion, accretion disks,novae, cataclysmic variables,stars: dwarf novae,stars: individual (EG Cancri)
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