A necessary condition for best fitting analytical to simulated density profiles in dark matter haloes

DOI10.1016/J.AMC.2005.04.088zbMath1089.85001arXivastro-ph/0501369OpenAlexW1976304046MaRDI QIDQ2490222

Roberto Caimmi

Publication date: 28 April 2006

Published in: Applied Mathematics and Computation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0501369

zbMATH Keywords

cosmologydark matterclustersgalaxiesgeneral

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)

Cites Work

• Density profile asymptotes at the centre of dark matter halos

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