Concentration, spin and shape of dark matter haloes as a function of the cosmological model:WMAP1, WMAP3 andWMAP5 results
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/391/4/1940/4902554/mnras0391-1940.pdf
Reference49 articles.
1. Dark Matter Properties and Halo Central Densities
2. The shape of dark matter haloes: dependence on mass, redshift, radius and formation
3. Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
4. Contraction of dark matter galactic halos due to baryonic infall
5. Profiles of dark haloes: evolution, scatter and environment
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