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Zenodo, 2017

DOI: 10.5281/zenodo.580566

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A Model For Black Hole Growth In The Local Universe

Journal article published in 2017 by Anna Weigel, Kevin Schawinski ORCID, Neven Caplar, Ivy Wong, Ezequiel Treister
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

Using a phenomenological model, black hole growth in the local Universe can be described by two separate, mass independent Eddington ratio distribution functions (ERDFs).

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