Hostname: page-component-6bf8c574d5-w79xw Total loading time: 0 Render date: 2025-02-28T04:42:58.681Z Has data issue: false hasContentIssue false
  • English
  • Français

Possibility of fluorescence phenomena in the ultraviolet spectrum of symbiotic stars and long period variables

Published online by Cambridge University Press:  14 August 2015

J. P. Swings  and
P. Swings
J. P. Swings
Affiliation:
Institut d'Astrophysique, Cointe-Ougrée, Belgium
P. Swings
Affiliation:
Institut d'Astrophysique, Cointe-Ougrée, Belgium

Abstract

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.

We discuss essentially the cases where molecular fluorescences may be excited by Lyman α and other strong discrete ultraviolet emissions, including lines beyond the Lyman limit. The stars involved are the symbiotic objects and the long period variables. The molecules are H2, N2, O2, NO and CO which have their resonance systems in the ultraviolet.

Type
Part II: Stellar Line Spectra
Information
Symposium - International Astronomical Union , Volume 36: Ultraviolet Stellar Spectra and Related Ground-Based Observations , 1970 , pp. 226 - 231
Copyright
Copyright © Reidel 1970 

References

Aller, L. H.: 1961, Mem. Soc. Roy. Sc. Liège 4, 535.Google Scholar
Moore, C. E.: 1952, A UV Multiplet Table, NBS Circ. 488.CrossRefGoogle Scholar
Simmons, J. D., Bass, A. M., and Tilford, S. G.: 1969, Astrophys. J. 155, 345.Google Scholar
Swings, P.: 1933, ‘Spectres moléculaires’, Act. Sc. Ind. 74, Paris, Hermann.Google Scholar
Swings, P.: 1965, ‘Astronautical Investigations of Comets’, in Advances in Space Science and Technology, Vol. 7 (ed. by Ordway, F. I. III), Academic Press, New York.Google Scholar