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UV time-dependent emission in SY Muscae
Published online by Cambridge University Press: 12 April 2016
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Ultraviolet spectra acquired with the International Ultraviolet Explorer (IUE) of SY Mus = HD 10036 on 20 September 1980 and 11 June 1981 indicate a substantial enhancement of UV emission over a nine month period. The general UV flux level appears to have increased by approximately one order of magnitude between the first and second observing epochs. The strong ultraviolet continuum evident throughout the entire IUE spectral range λλ1200-3200 A on 11 June 1981 is closely approximated by a star with Teff = 40,000 K, where previously on 20 September 1980 the continuum distribution presented a more complex structure that is possibly explained by a combination of thermal emission from an early type main sequence star, and nebular recombination emission (Michalitsianos et al. 1981).
- Type
- Session II – Discussion on Individual Stars
- Information
- International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 191 - 194
- Copyright
- Copyright © Reidel 1982
References
Altamore, A., Baratta, G.B., Cassatella, A., Freidjung, M., Giangrande, A., Ricciardi, O. and Viotti, R.
1981, Astrophys. J., 245, p. 630.Google Scholar
Kafatos, M., Michalitsianos, A.G. and Hobbs, R.W.
1980, Astropnys. J., 240, p. 114.CrossRefGoogle Scholar
Michalitsianos, A.G., Kafatos, M., Feibelman, W.A. and Hobbs, R.W.
1981, Astropnys. J., in press.Google Scholar
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