Abstract
Nova Vul 1984 n°2 has been again observed at Observatoire de Haute-Provence in the autumn of 1985, i.e. 270-295 days after maximum. It was then in the nebular phase. The spectra cover the blue-violet and the near infrared regions. Over 50 lines and blends have been identified and are given in Table 2. No clear pattern is observed in the emission bands of a width of about 1450 km/sec. The most conspicuous features observed are the forbidden NeIII and NeV lines. The infrared region is dominated by a very strong He I 1083nm emission.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Andrillat Y. and Houziaux L., 1985 Recent Results on Cataclysmic Variables, Bamberg, ESA-SP 236, 187–191.
Gehrz R.D., Grasdalen G.L. and Hackwell J.A., 1985 Astrophys. J. 298, L47-L51.
Schweitzer E., 1986 IAU Circ. n° 4164.
Starrfield S., Sparks W.M. and Truran J.W., 1986 Astrophys. J. 303, L5-L9.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1987 D. Reidel Publishing Company
About this paper
Cite this paper
Andrillat, Y., Houziaux, L. (1987). The Spectrum of Nova Vulpeculae 1984 N°2 at Nebular Phase. In: Drechsel, H., Kondo, Y., Rahe, J. (eds) Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3801-4_67
Download citation
DOI: https://doi.org/10.1007/978-94-009-3801-4_67
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8191-7
Online ISBN: 978-94-009-3801-4
eBook Packages: Springer Book Archive