Spectroscopic and Photometric follow-up of MASTER OT J030227.28+191754.5
We performed spectroscopic and photometric observations. We propose that this object is a possible narrow-lined He nova or very large-amplitude WZ Sge-type dwarf nova. https://www.astronomerstelegram.org/?read=15072
This object is showing enigmatic behavior. Further observations are strongly encouraged!
vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp