30 Sep
2022
30 Sep
'22
10:29 p.m.
TCPJ23580961+5502508: new WZ Sge-type dwarf nova
Kyoto Univ. Obs. observed TCPJ23580961+5502508 on 30th Sep. We detected early superhumps with a period of ~0.060 d, and an amplitude of 0.2 mag! Therefore TCPJ23580961+5502508 is a new WZ Sge-type dwarf nova, and also has one of the largest early superhump amplitude.
Follow-up photometry is strongly encouraged. Best,Yusuke
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Kyoto University, Graduate School of Department of Astronomy, PhD student
Yusuke TAMPO
MAIL: tampo@kusastro.kyoto-u.ac.jp
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