The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores (2014)

First Author: Di Cintio A
Attributed to:  An Astrophysics Consolidated Grant for the Jeremiah Horrocks Institute funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stt1891

Publication URI: http://dx.doi.org/10.1093/mnras/stt1891

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1