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]
S. K. Ballero, F. Matteucci, L. Ciotti (2008). Chemical evolution of Seyfert galaxies. CAMBRIDGE : Cambridge University Press.
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:
Eventuali allegati, non sono esposti
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
