Empirical Models for Dark Matter Halos. III. The Kormendy Relation and the log ρ e -log R e Relation
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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
| Collections | ANU 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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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Graham_Empirical_Models_for_Dark_2006.pdf | 266.77 kB | Adobe PDF | Request a copy |
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