Evidences for the Development of a Collisional Spectrum in the Nebular Stage of Novae
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.
KeywordsPublishing Company Radiative Ionization Spectroscopical Data Filling Factor Alternative Interpretation
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© D. Reidel Publishing Company, Dordrecht, Holland 1977