TCP J07363658+4151215: most likely helium WZ Sge-type dwarf nova
Kyoto U. team has reported observations. The data show early superhumps with an amplitudes of 0.05 mag. The period is 0.0280(2) d. This object is most likely a helium WZ Sge star. The SDSS color (very blue u-g=+0.27) is consistent.
Kyoto U. team spectroscopically observed this object by the 3.8m-telescope Seimei. The object shows Hbeta and gamma absorption lines, so the object is not helium-rich. However, this object will be a WZ Sge star, and hence it is worth observing. Continuous photometry is encouraged.
On 2021/11/05 9:37, Taichi Kato wrote:
TCP J07363658+4151215: most likely helium WZ Sge-type dwarf nova
Kyoto U. team has reported observations. The data showearly superhumps with an amplitudes of 0.05 mag. The period is 0.0280(2) d. This object is most likely a helium WZ Sge star. The SDSS color (very blue u-g=+0.27) is consistent.
vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp
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Keisuke Isogai -
Taichi Kato