We computed the chemical evolution of Seyfert galaxies, residing in spiral bulges, based on an updated model for the Milky Way bulge with updated calculations of the Galactic potential and of the feedback from the central supermassive black hole (BH) in a spherical approximation. [Abridged]
Chemical evolution of Seyfert galaxies / S. K. Ballero; F. Matteucci; L. Ciotti. - STAMPA. - (2008), pp. 231-232. (Intervento presentato al convegno IAU Symposium 245, Formation and evolution of galaxy bulges tenutosi a Oxford, UK nel 16-20 luglio 2007).
Chemical evolution of Seyfert galaxies
CIOTTI, LUCA
2008
Abstract
We computed the chemical evolution of Seyfert galaxies, residing in spiral bulges, based on an updated model for the Milky Way bulge with updated calculations of the Galactic potential and of the feedback from the central supermassive black hole (BH) in a spherical approximation. [Abridged]File in questo prodotto:
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