M. Dellavalle et al., STUDY OF NOVA SHELLS .2. FH SERENTIS-1970 AND QU VULPECULAE-1984, NEBULAR EXPANSION, PARALLAX AND LUMINOSITY, Astronomy and astrophysics, 325(3), 1997, pp. 1151-1156
We present H alpha direct imaging and shell spectroscopic observations
of two classical novae: FH Ser 1970 and QU Vul 1984. The distances, r
eddenings, luminosities at maximum, and the mass of the shell ejected
by FH Ser are derived and discussed.