Black hole spin and radio loudness in a Λ cold dark matter universe

We use a combination of a cosmological N-body simulation of the concordance Λ cold dark matter paradigm and a semi-analytic model of galaxy formation to investigate the spin development of central supermassive black holes (BHs) and its relation to the BH host galaxy properties. In order to compute B...

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Detalles Bibliográficos
Autores principales: Lagos, Claudia del Pilar, Padilla, Nelson D., Cora, Sofía Alejandra
Formato: Articulo
Lenguaje:Inglés
Publicado: 2009
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82680
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