Results 111 to 120 of about 617 (181)

Halo Asymmetry in the Modeling of Galaxy Clustering

open access: yesThe Astrophysical Journal
Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter halos can be approximated by the Navarro–Frenk–White (NFW) spherically symmetric profile.
Anna Durkalec   +2 more
doaj   +1 more source

Linking Warm Dark Matter to Merger Tree Histories via Deep Learning Networks

open access: yesThe Astrophysical Journal
Dark matter (DM) halos form hierarchically in the Universe through a series of merger events. By pairing halo finder and postprocessing codes, merger series in cosmological simulations can be conveniently represented as a graph-like “tree” structure ...
Ilem Leisher   +13 more
doaj   +1 more source

The Formation of Dark Matter Halos and High-Redshift Galaxies

open access: yes, 2011
In the concordance LCDM cosmological model, galaxies form in the centers of dark matter halos and merge with one another following the mergers of their host halos. Thus, we set out to quantify the growth mechanisms of dark matter halos. For this purpose, we analyze several large N-body simulations of the growth of cosmic structure.
openaire   +2 more sources

The era of precision cosmology with voids. [PDF]

open access: yesAstron Astrophys Rev
Contarini S, Verza G, Pisani A.
europepmc   +1 more source

The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]

open access: yesNature
Taylor ED   +9 more
europepmc   +1 more source

Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [PDF]

open access: yesNature, 2023
Di Mascolo L   +15 more
europepmc   +1 more source

Simulations of multi-phase gas in and around galaxies. [PDF]

open access: yesLiving Rev Comput Astrophys
Gronke M, E Schneider E.
europepmc   +1 more source

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