Study of nova shells .2. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity

Della Valle M., Gilmozzi R., Bianchini A., Esenoglu H. H.

ASTRONOMY & ASTROPHYSICS, cilt.325, sa.3, ss.1151-1156, 1997 (SCI-Expanded) identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 325 Sayı: 3
  • Basım Tarihi: 1997
  • Dergi Adı: ASTRONOMY & ASTROPHYSICS
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.1151-1156
  • Anahtar Kelimeler: galaxies, individual, NGC 1380, novae, cataclysmic variables, stars, distances, CLASSICAL NOVAE, DISTANCE
  • İstanbul Üniversitesi Adresli: Evet

Özet

We present H alpha 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.
We present Hαdirect imaging and shell spectro-
scopic observations of two classical novae: FH Ser 1970 and
QU Vul 1984. The distances, reddenings, luminosities at max-
imum, and the mass of the shell ejected by FH Ser are derived
and discussed.