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)
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