Results 11 to 20 of about 10,749 (290)

Determining Omega from Peculiar Velocities [PDF]

open access: green, 1993
9 pages including 6 figures, compressed and uuencoded PostScript 0.6Mbyte, for Cosmic Velocitiy Fields, IAP Paris July 1993 (preprint: HUJI-AST-002) (Also available by anonymous ftp from alf.huji.ac.il as pub/dekel/reviews/iap93.ps.Z of 0.44Mbyte)
Avishai Dekel
openalex   +3 more sources

Are Recent Peculiar Velocity Surveys Consistent? [PDF]

open access: green, 1999
We compare the bulk flow of the SMAC sample to the predictions of popular cosmological models and to other recent large-scale peculiar velocity surveys. Both analyses account for aliasing of small-scale power due to the sparse and non-uniform sampling of the surveys.
Michael J. Hudson   +4 more
openalex   +5 more sources

Deep Learning nearby galaxy peculiar velocities [PDF]

open access: green, 2022
9 pages, 5 figures, submitted to ...
Kevin M. Quigley   +2 more
openalex   +3 more sources

HVS 7: a chemically peculiar hyper-velocity star [PDF]

open access: bronzeAstronomy & Astrophysics, 2008
Context: Hyper-velocity stars are suggested to originate from the dynamical interaction of binary stars with the supermassive black hole in the Galactic centre (GC), which accelerates one component of the binary to beyond the Galactic escape velocity. Aims: The evolutionary status and GC origin of the HVS SDSS J113312.12+010824.9 (HVS7) is constrained ...
N. Przybilla   +5 more
openalex   +3 more sources

Peculiar Velocities of Galaxy Clusters [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 1998
8 pages, 4 figures; submitted to ...
J. M. Colberg   +7 more
openalex   +4 more sources

Modelling peculiar velocities of dark matter haloes [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2003
We present a simple model that accurately describes various statistical properties of peculiar velocities of dark matter halos. We pay particular attention to the following two effects; first, the evolution of the halo peculiar velocity depends on the local matter density, instead of the global density.
Takashi Hamana   +4 more
openalex   +5 more sources

Wide-angle effects for peculiar velocities [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT The line-of-sight peculiar velocities of galaxies contribute to their observed redshifts, breaking the translational invariance of galaxy clustering down to a rotational invariance around the observer. This becomes important when the line-of-sight direction varies significantly across a survey, leading to what are known as ‘wide-
Emanuele Castorina, Martin White
openaire   +5 more sources

The peculiar velocity correlation function [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
We present an analysis of the two-point peculiar velocity correlation function using data from the CosmicFlows catalogues. The Millennium and MultiDark Planck 2 N-body simulations are used to estimate cosmic variance and uncertainties due to measurement errors. We compare the velocity correlation function to expectations from linear theory to constrain
Wang, Yuyu   +3 more
openaire   +2 more sources

Peculiar velocities in the early Universe

open access: yesPhysical Review D, 2022
Typos corrected.
Myrto Maglara, Christos G. Tsagas
openaire   +2 more sources

Infall from peculiar velocities [PDF]

open access: yesProceedings of the International Astronomical Union, 2004
We perform a statistical analysis to study the infall of galaxies onto groups and clusters in the nearby Universe. The study is based on the UZC/SSRS2 group catalogs and galaxy peculiar velocity data. We find a clear signature of infall of galaxies onto groups in a large range of scales 5 Mpc h−1 < r < 30 Mpc h−1.
María Laura Ceccarelli   +5 more
openaire   +1 more source

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