Dear colleagues, Is anyone able to get spectroscopy during the current outburst of UW Tri? We would like to know whether this object is a recurrent nova or a peculiar dwarf nova. Although we would favor the latter, the light curve obtained at Ouda shows a steady decline with a rate of 0.2 mag/day, which is rather atypical for familiar types of dwarf novae, but may be interpreted as a fast nova with t3=15d. Best regards, Daisaku Nogami