Abstract
In the frame of the Starburst Model, we show that the evolution of a massive stellar cluster in a high metallicity environment can reproduce the observed emission-line spectrum and the UV-optical Spectral Energy Distribution of the Seyfert 2 galaxies and LINERs. We apply the results of our models to three objects: NGC 5506, NGC 5643 and Mk 348.
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Vargas, M.L.G., Díaz, A., Terlevich, R., Terlevich, E. (1993). Testing the Consistency of the Starburst Scenario for Active Galactic Nuclei. In: Beckman, J.E. (eds) The Nearest Active Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1930-6_12
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DOI: https://doi.org/10.1007/978-94-011-1930-6_12
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