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Empirical Models for Dark Matter Halos. III. The Kormendy Relation and the log ρ e -log R e Relation

Graham, Alister; Merritt, David; Moore, Ben; Diemand, Jürg; Terzic, Balsa

Description

We have recently shown that the three-parameter density profile model from Prugniel & Simien provides a better fit to simulated galaxy- and cluster-sized dark matter halos than an Navarro-Frenk-White-like model with arbitrary inner profile slope 7 (Paper

CollectionsANU Research Publications
Date published: 2006
Type: Journal article
URI: http://hdl.handle.net/1885/30894
Source: Astronomical Journal
DOI: 10.1086/508992

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