Study of nova shells. II. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity.

Details Study of nova shells. II. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity. Study of nova shells. II. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...325.1151d&link_type=abstract

Astronomy and Astrophysics, v.325, p.1151-1156

Astronomy and Astrophysics

Astrophysics

14

Galaxies: Individual: Ngc 1380, Novae: Cataclysmic Variables, Stars: Distances

Scientific paper

We present Hα direct imaging and shell spectroscopic observations
of two classical novae: FH Ser 1970 and QU Vul 1984. The distances,
reddenings, luminosities at maximum, and the mass of the shell ejected
by FH Ser are derived and discussed.

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