Evidences for the Development of a Collisional Spectrum in the Nebular Stage of Novae

  • Y. Andrillat
  • S. Collin-Souffrin
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 65)


The study of the coronal lines of [FeX] and [FeXIV] in the spectrum of Nova Ophiuchi 1958, Nova Herculis 1963, Nova Delphini 1967, shows that a very thin and hot (≳ 106 K) region develops in the envelope.


Publishing Company Radiative Ionization Spectroscopical Data Filling Factor Alternative Interpretation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


  1. Aller, L., Kayes, C. 1974, Astrophys. Spa. Sci, 30, 387.ADSCrossRefGoogle Scholar
  2. Mc Laughlin, D.B. 1949, Publ. Obs. Michigan, 9, 13.ADSGoogle Scholar
  3. Nussbaumer, H., Osterbrock, D.E. 1970, Astrophys,J. 161, 81.ADSCrossRefGoogle Scholar
  4. Pottasch, S.R. 1967, Bull. Astron. Inst. Neth, 19, 227.ADSGoogle Scholar
  5. Swing, P., Jose, P.D. 1949, Astrophys,J. 110, 475.ADSCrossRefGoogle Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1977

Authors and Affiliations

  • Y. Andrillat
    • 1
    • 2
  • S. Collin-Souffrin
    • 1
    • 2
  1. 1.Observatoire de Haute ProvenceForcalquierFrance
  2. 2.Observatoire de MeudonD.A.F.MeudonFrance

Personalised recommendations