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First Detection of Two Superoutbursts During the Rebrightening Phase of a WZ Sge-type Dwarf Nova: TCP J21040470+4631129

Yusuke Tampo,Kojiguchi Naoto,Keisuke Isogai,Taichi Kato,Mariko Kimura,Yasuyuki Wakamatsu,Daisaku Nogami,Tonny Vanmunster,Tamas Tordai,Hidehiko Akazawa, Felipe Mugas,Taku Nishiumi,Victor J. S. Bejar,Kiyoe Kawauchi,Nicolas Crouzet,Noriharu Watanabe,Nuria Casasayas-Barris,Yuka Terada,Akihiko Fukui,Norio Narita,Enric Palle,Motohide Tamura,Nobuhiko Kusakabe,Roi Alonso,Hiroshi Itoh,Kirill Sokolovsky, Brandon McIntyre,Jesse Leahy-McGregor,Stephen M. Brincat,Pavol A. Dubovsky,Tomas Medulka,Igor Kudzej,Elena P. Pavlenko,Kirill A. Antonyuk,Nikolaj Pit,Oksana Antonyuk,Julia Babina,Aleksei Baklanov, Aleksander S. Sklyanov,Alexandra M. Zubareva,Aleksandr A. Belinski, Alexandr Dodin,Marina A. Burlak,Natalia P. Ikonnikova,Egor O. Mishin,Sergey A. Potanin,Ian Miller,Michael Richmond,Roger D. Pickard,Charles Galdies,Masanori Mizutani,Kenneth Menzies,Geoffrey Stone,Javier Ruiz

Publications of the Astronomical Society of Japan（2020）

引用 14|浏览61
关键词
accretion, accretion disk,novae, cataclysmic variables,stars: dwarf novae,stars: individual (TCP J21040470+4631129)
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