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!
MASTER OT J030227.28+191754.5 211129.0829 12.0V FID
The photomerty was based on a 60s image with V-band filter, using an 0.25m iTelescope.net reflector remotely at Mayhill, New Mexico, US, using APASS V magnitudes.
Photo (with preliminary photometry): https://twitter.com/fidusz/status/1465190900812947456
Róbert Fidrich HAA/VSS Budakeszi, Hungary
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp