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A Mass Dependent Density Profile from Dwarfs to Clusters

In this paper, we extend the work of Freundlich et al. 2020 who showed how to obtain a Dekel–Zhao density profile with mass dependent shape parameters in the case of galaxies. In the case of Freundlich et al. 2020, the baryonic dependence was obtained using the NIHAO set of simulations. In our case,...

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Detalles Bibliográficos
Principais autores: Antonino Del Popolo, Morgan Le Delliou
Formato: Artigo
Idioma:Inglês
Publicado: MDPI AG 2022-05-01
Series:Galaxies
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Acceso en liña:https://www.mdpi.com/2075-4434/10/3/69
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