Results 81 to 90 of about 427,202 (211)

Shock‐heated Gas in the Large‐Scale Structure of the Universe [PDF]

open access: bronze, 2005
HyeSung Kang   +7 more
openalex   +1 more source

Two-dimensional simulation of the gravitational system dynamics and formation of the large-scale structure of the Universe [PDF]

open access: bronze, 1980
А. G. Doroshkevich   +5 more
openalex   +1 more source

Emulating Power Spectra for Prereconstructed and Postreconstructed Galaxy Samples

open access: yesThe Astrophysical Journal
The small-scale linear information in galaxy samples typically lost during nonlinear growth can be restored to a certain level by the density field reconstruction, which has been demonstrated for improving the precision of the baryon acoustic oscillation
Yuting Wang   +12 more
doaj   +1 more source

Orthogonal Alignment of Galaxy Group Angular Momentum with Cosmic Filament Spines: An Observational Study

open access: yesThe Astrophysical Journal Letters
We investigated the alignment between the angular momenta of galaxy groups and the spines of their associated cosmic filaments. Our results demonstrate a significant tendency for these two orientations to be perpendicular, indicating that the rotation of
Yu Rong, Peng Wang, Xiao-xiao Tang
doaj   +1 more source

DarkAI: Reconstructing the Density, Velocity, and Tidal Fields of Dark Matter from a DESI-like Bright Galaxy Sample

open access: yesThe Astrophysical Journal Supplement Series
Reconstructing the mass density, velocity, and tidal (MTV) fields of dark matter from galaxy surveys is essential for advancing our understanding of the large-scale structure of the Universe.
Feng Shi   +12 more
doaj   +1 more source

Cosmic Tidal Reconstruction in Redshift Space

open access: yesThe Astrophysical Journal
Gravitational coupling between large- and small-scale density perturbations leads to anisotropic distortions to local small-scale matter fluctuations. Such local anisotropic distortions can be used to reconstruct large-scale matter distribution, known as
Shi-Hui Zang   +3 more
doaj   +1 more source

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

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