Active galactic nuclei at z ~ 1.5: I. Spectral energy distribution and accretion discs

The physics of active super massive black holes (BHs) is governed by their mass (M_BH), spin (a*) and accretion rate (\(\dot{M}\)). This work is the first in a series of papers with the aim of testing how these parameters determine the observable attributes of active galactic nuclei (AGN). We have s...

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Veröffentlicht in:	arXiv.org 2014-10
Hauptverfasser:	Capellupo, Daniel M, Netzer, Hagai, Lira, Paulina, Trakhtenbrot, Benny, Mejía-Restrepo, Julían
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Active galactic nuclei Bayesian analysis Biological evolution Deposition Mathematical models Milky Way Galaxy Parameters Physics - Astrophysics of Galaxies Red shift Spectral energy distribution Stellar winds
Online-Zugang:	Volltext
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