T Cor B, a “Seyfert 1 Nucleus” at 1200±100 Parsecs?
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.
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