Results 21 to 30 of about 113,786 (346)
Caustics in dark matter haloes [PDF]
EAS Publications Series, 2006 Comment: Minor changes, two references added, 6 pages, 3 figures, to appear in Proc. 21st IAP Colloquium "Mass Profiles and Shapes of Cosmological Structures", Paris 4-9 July 2005, [EAS Publications Series, eds: G. Mamon, F. Combes, C. Deffayet, B. Fort]
Roya Mohayaee +5 more
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Scale Lengths in Dark Matter Halos [PDF]
The Astrophysical Journal, 2005 We investigate a hypothesis regarding the origin of the scalelength in halos formed in cosmological N-body simulations. This hypothesis can be viewed as an extension of an earlier idea put forth by Merritt and Aguilar. Our findings suggest that a phenomenon related to the radial orbit instability is present in such halos and is responsible for density ...
Arif Babul +5 more
openaire +3 more sources
The total mass of dark matter haloes [PDF]
Monthly Notices of the Royal Astronomical Society, 2011 7 pages, 6 figures.
Anderhalden D, Diemand J
openaire +5 more sources
Symposium - International Astronomical Union, 1996 The observational evidence for dark halos around galaxies is shortly reviewed. New and old techniques and results constraining the mass, the distribution, the shape and the nature of dark halos are discussed.
openaire +2 more sources
The abundance of (not just) dark matter haloes [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 19 pages, updated version published in ...
Carlos S. Frenk +8 more
openaire +7 more sources
A New Stellar Mass Proxy for Subhalo Abundance Matching
The Astrophysical Journal, 2023 Subhalo abundance matching (SHAM) has played an important role in improving our understanding of how galaxies populate their host dark matter halos.
Chen-Yu Chuang, Yen-Ting Lin
doaj +1 more source
Analytic model for galaxy and dark matter clustering [PDF]
, 2000 We investigate an analytic model to compute nonlinear power spectrum of dark matter, galaxies and their cross-correlation. The model is based on Press-Schechter halos, which cluster and have realistic dark matter profiles.
Spergel, U. Seljak
core +2 more sources
WEIGHING THE DARK MATTER HALO [PDF]
The Identification of Dark Matter, 2005 6 pages, 2 figures. To appear in "IDM2004: The 5th International Workshop on the Identification of Dark Matter", eds. N.
openaire +3 more sources
Substructures in cold dark matter haloes [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 We analyse the properties of substructures within dark matter halos (subhalos) using a set of high-resolution numerical simulations of the formation of structure in a Lambda-CDM Universe. Our simulation set includes 11 high-resolution simulations of massive clusters as well as a region of mean density, allowing us to study the spatial and mass ...
De Lucia G. +7 more
openaire +6 more sources
Properties of dark matter haloes [PDF]
New Astronomy Reviews, 2002 An overview is presented of the main properties of dark matter haloes, as we know them from observations, essentially from rotation curves around spiral and dwarf galaxies. Detailed rotation curves are now known for more than a thousand galaxies, revealing that they are not so flat in the outer parts, but rising for late-types, and falling for early ...
openaire +4 more sources