Raj, A; Pavana, M; Kamath, U. S; Anupama, G. C; Walter, F. M
(Copernicus Foundation for Polish Astronomy, 2018-03)
Using our previously reported observations, we derive some physical parameters of the moderately fast nova V2676 Oph 2012 #1. The best-fit CLOUDY model of the nebular spectrum obtained
on 2015 May 8 shows a hot white dwarf ...