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The dependence of dark matter profiles on the...
Preprint

The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Abstract

We use 31 simulated galaxies from the MaGICC project to investigate the effects of baryonic feedback on the density profiles of dark matter (DM) haloes. The sample covers a wide mass range: 9.4e9

Authors

Di Cintio A; Brook CB; Maccio AV; Stinson GS; Knebe A; Dutton AA; Wadsley J

Publication date

June 4, 2013

DOI

10.48550/arxiv.1306.0898

Preprint server

arXiv
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