Formation and feeding of supermassive black holes in the early universe

Details Formation and feeding of supermassive black holes in the early universe Formation and feeding of supermassive black holes in the early universe

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222..519d&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Physics

Scientific paper

We present a physical and numerical model of accretion driven growth of super-massive black holes. In this model we can account for (a) the existence of > 109 M&sun; black holes already in the first quasars and (b) for the observation that the lower luminosity AGN distribution peaks later in the evolution of the Universe than that of more luminous objects.

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