A mass-dependent density profile for dark matter haloes including the influence of galaxy formation-Reference-Cited by-同舟云学术

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A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

Published:2014-05-24 Issue:4 Volume:441 Page:2986-2995
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Cintio Arianna Di,Brook Chris B.,Dutton Aaron A.,Macciò Andrea V.,Stinson Greg S.,Knebe Alexander

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/441/4/2986/4040058/stu729.pdf

Reference81 articles.

1. Fundamental differences between SPH and grid methods

2. The radial velocity dispersion profile of the Galactic halo: constraining the density profile of the dark halo of the Milky Way

3. Contraction of dark matter galactic halos due to baryonic infall

4. Hierarchical formation of bulgeless galaxies - II. Redistribution of angular momentum via galactic fountains

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