Results 11 to 20 of about 10,749 (290)
Determining Omega from Peculiar Velocities [PDF]
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
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Are Recent Peculiar Velocity Surveys Consistent? [PDF]
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
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Deep Learning nearby galaxy peculiar velocities [PDF]
9 pages, 5 figures, submitted to ...
Kevin M. Quigley +2 more
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HVS 7: a chemically peculiar hyper-velocity star [PDF]
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
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Peculiar Velocities of Galaxy Clusters [PDF]
8 pages, 4 figures; submitted to ...
J. M. Colberg +7 more
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Modelling peculiar velocities of dark matter haloes [PDF]
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
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Wide-angle effects for peculiar velocities [PDF]
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
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The peculiar velocity correlation function [PDF]
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
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Peculiar velocities in the early Universe
Typos corrected.
Myrto Maglara, Christos G. Tsagas
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Infall from peculiar velocities [PDF]
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
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