[vsnet-outburst 24768] TCP J15305274-0405572: SU UMa star confirmed
Taichi Kato
tkato at kusastro.kyoto-u.ac.jp
Fri Mar 6 09:14:07 JST 2020
TCP J15305274-0405572: SU UMa star confirmed
Based on the most recent data (Mar. 4) by Berto Monard,
superhumps with a mean amplitude of 0.21 mag were
confirmed. The period from this single-night observation
was 0.0601(3) d.
The short waiting time before the appearance
of ordinary superhumps and the large superhump
amplitude favor an ordinary SU UMa-type dwarf nova
rather than an extreme WZ Sge star despite
the large outburst amplitude.
More data are required whether this object
may show WZ Sge-type characteristics.
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