Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-02T22:18:04.023Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectral Peculiarities in Nova Vulpeculae 1984 N° 2

Published online by Cambridge University Press:  12 April 2016

Yvette Andrillat  and
Léo Houziaux
Yvette Andrillat
Affiliation:
Laboratoire d’Astronomie, Université des Sciences et Techniques du Languedoc, Montpellier, France.
Léo Houziaux
Affiliation:
Département d’Astrophysique, Université de Mons, Mons, Belgium.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This slow nova has been observed spectroscopically at Observatoire de Haute-Provence in two wavelengths regions: 330–460 nm (plate factors: 4 and 8 nm), and 750–1100 nm (plate factors: 23 and 26 nm/mm).

Time coverage includes the following stages: close to maximum of light, early nebular phase and advanced nebular stage.

Spectra are similar to those of classical novae: strong continuum, wide emission bands with double structure, flanked by a moderate strength absorption component at −1400 km/s.The following ions are identified: H I, O I, C I, N I, Mg I and II, Ca I and II, Fe II, Ti II, Si II and Sr II.

Type
Part III. Chemical and Dynamical Structures of Exploding Stars
Information
International Astronomical Union Colloquium , Volume 108: Atmospherics Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion , 1988 , pp. 232 - 233
Copyright
Copyright © Springer-Verlag 1988