Abstract
Several symbiotic stars are characterized by UV spectral signatures which are similar, in several aspects, to those observed in the broad-line region of Seyfert galaxies. We suggest to consider the symbiotic stars as a convenient laboratory for the study of the spectroscopic mechanisms which are at work in Seyfert 1 nuclei.
Based on observations by the International Ultraviolet Explorer (IUE) collected at the Villafranca Satellite Tracking Station (VILSPA) of the European Space Agency.
Affiliated to the Astrophysics Division, Space Sciences Department.
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© 1986 Springer Science+Business Media Dordrecht
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Selvelli, P.L., Clavel, J., Cassatella, A., Hack, M. (1986). T Cor B, a “Seyfert 1 Nucleus” at 1200±100 Parsecs?. In: Giuricin, G., Mardirossian, F., Mezzetti, M., Ramella, M. (eds) Structure and Evolution of Active Galactic Nuclei. Astrophysics and Space Science Library, vol 121. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4562-3_81
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DOI: https://doi.org/10.1007/978-94-009-4562-3_81
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