Abstract
Observations of the recetly discovered jet feature in the symbiotic variable R Aquarii (M7e=pec) were obtained with the International Ultraviolet Explorer (IUE). A comaparison of low dispersion UV-spectra reveals important differences between the central ionized source and the jet feature. The UV-continum flux Fλ between 1200-2000A that rises with decreasing wavelegth in the jet feature, essentially is independent with wavelength in the central compact nebula. The prominent emission lines of Si III] λ 1892A amd Si II λ 1817A, evident in the central star, are virtually absent in the jet. The carbon lines of C IV, C III] and C II also suggest the general excitation of the jet is comparatively lower than the central star. This is further indicated by enhanced S II λ 1250, 1295A and C II λ 1335A emission in the feature. We speculate that material that is ejected from the symbiotic system cools through free-free and nebular recombination emission.
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References
Bath G.T., and Pringle, J.E.:1982,M.N.R.A.S., in press.
Boyarchuk,“?:lk iiii .A.A.:1982,“The Nature of Symbiotic Stars”, edit. M.Friedjung and R. Viotti (D.Reidel Publishing Co.),pp.225–230.
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References
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© 1983 International Astronomical Union
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Michalitsianos, A.G. et al. (1983). Joint Commission Meeting on UV and X-Ray Observations of Interacting Binary Systems. In: West, R.M. (eds) Highlights of Astronomy. International Astronomical Union / Union Astronomique Internationale, vol 6. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7110-3_12
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DOI: https://doi.org/10.1007/978-94-009-7110-3_12
Publisher Name: Springer, Dordrecht
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