The coherence length of the peculiar velocity field in the universe and the large-scale galaxy correlation data

1992 ◽  
Vol 386 ◽  
pp. L37 ◽  
Author(s):  
A. Kashlinsky
Keyword(s):  
Velocity Field ◽  
Coherence Length ◽  
Large Scale ◽  
Peculiar Velocity ◽  
Correlation Data ◽  
The Universe

scholarly journals The large-scale peculiar velocity field in flat models of the universe

1987 ◽  
Vol 316 ◽  
pp. 475 ◽  
Author(s):  
Nicola Vittorio ◽  
Michael S. Turner
Keyword(s):  
Velocity Field ◽  
Large Scale ◽  
Peculiar Velocity ◽  
The Universe

scholarly journals A slight excess of large-scale power from moments of the peculiar velocity field

2011 ◽  
Vol 414 (1) ◽  
pp. 621-626 ◽  
Author(s):  
E. Macaulay ◽  
H. Feldman ◽  
P. G. Ferreira ◽  
M. J. Hudson ◽  
R. Watkins
Keyword(s):  
Velocity Field ◽  
Large Scale ◽  
Peculiar Velocity ◽  
Slight Excess

scholarly journals A kinematic confirmation of the hidden Vela supercluster

2019 ◽  
Vol 490 (1) ◽  
pp. L57-L61 ◽  
Author(s):  
Hélène M Courtois ◽  
Renée C Kraan-Korteweg ◽  
Alexandra Dupuy ◽  
Romain Graziani ◽  
Noam I Libeskind
Keyword(s):  
Excellent Agreement ◽  
Mass Concentration ◽  
Large Scale ◽  
Milky Way ◽  
Large Scale Structure ◽  
Peculiar Velocity ◽  
The Galaxy ◽  
Zone Of Avoidance ◽  
First Time ◽  
The Universe

ABSTRACT The Universe region obscured by the Milky Way is very large and only future blind large H i redshift, and targeted peculiar surveys on the outer borders will determine how much mass is hidden there. Meanwhile, we apply for the first time two independent techniques to the galaxy peculiar velocity catalogue CosmicFlows−3 in order to explore for the kinematic signature of a specific large-scale structure hidden behind this zone: the Vela supercluster at cz ∼18 000 km s−1. Using the gravitational velocity and density contrast fields, we find excellent agreement when comparing our results to the Vela object as traced in redshift space. The article provides the first kinematic evidence of a major mass concentration (knot of the Cosmic Web) located in the direction behind Vela constellation, pin pointing that the Zone of Avoidance should be surveyed in detail in the future.

scholarly journals Spiral Galaxies and the Peculiar Velocity Field

1996 ◽  
Vol 168 ◽  
pp. 183-191 ◽  
Author(s):  
Riccardo Giovanelli ◽  
Martha P. Haynes ◽  
Pierre Chamaraux ◽  
Luiz N. Da Costa ◽  
Wolfram Freudling ◽  
...  
Keyword(s):  
Velocity Field ◽  
Reference Frame ◽  
Large Scale ◽  
Local Group ◽  
Spiral Galaxies ◽  
Density Parameter ◽  
Compelling Evidence ◽  
Homogeneous Sample ◽  
Peculiar Velocity ◽  
Peculiar Velocities

We report results of a redshift-independent distance measurement survey that extends to all sky and out to a redshift of approximately 7500 km s−1. Tully–Fisher (TF) distances for a homogeneous sample of 1600 late spiral galaxies are used to analyze the peculiar velocity field. We find large peculiar velocities in the neighborhood of superclusters, such as Perseus–Pisces (PP) and Hydra–Centaurus, but the main clusters embedded in those regions appear to be virtually at rest in the CMB reference frame. We find no compelling evidence for large-scale bulk flows, whereby the Local Group, Hydra–Cen and PP would share a motion of several hundred km s−1with respect to the CMB. Denser sampling in the PP region allows a clear detection of infall and backflow motions, which can be used to map the mass distribution in the supercluster and to obtain an estimate of the cosmological density parameter.

scholarly journals Large-scale peculiar velocities through the galaxy luminosity function at z ~ 0.1

2014 ◽  
Vol 11 (S308) ◽  
pp. 332-335
Author(s):  
Martin Feix ◽  
Adi Nusser ◽  
Enzo Branchini
Keyword(s):  
Velocity Field ◽  
Large Scale ◽  
Zero Point ◽  
Peculiar Velocity ◽  
Peculiar Velocities ◽  
The Galaxy ◽  
Linear Velocity Field ◽  
Density Perturbations ◽  
Velocity Moments ◽  
Galaxy Luminosity Function

AbstractPeculiar motion introduces systematic variations in the observed luminosity distribution of galaxies. This allows one to constrain the cosmic peculiar velocity field from large galaxy redshift surveys. Using around half a million galaxies from the SDSS Data Release 7 at z ~ 0.1, we demonstrate the applicability of this approach to large datasets and obtain bounds on peculiar velocity moments and σ8, the amplitude of the linear matter power spectrum. Our results are in good agreement with the ΛCDM model and consistent with the previously reported ~ 1% zero-point tilt in the SDSS photometry. Finally, we discuss the prospects of constraining the growth rate of density perturbations by reconstructing the full linear velocity field from the observed galaxy clustering in redshift space.

scholarly journals Relativistic approach to the kinematics of large-scale peculiar motions

2020 ◽  
Vol 80 (8) ◽  
Author(s):  
Eleni Tsaprazi ◽  
Christos G. Tsagas
Keyword(s):  
Velocity Field ◽  
Growth Rates ◽  
Large Scale ◽  
Cosmological Perturbation ◽  
Cosmological Perturbation Theory ◽  
Peculiar Velocity ◽  
Linear Evolution ◽  
Peculiar Velocities ◽  
Bulk Motion ◽  
Relativistic Approach

Abstract We consider the linear kinematics of large-scale peculiar motions in a perturbed Friedmann universe. In so doing, we take the viewpoint of the “real” observers that move along with the peculiar flow, relative to the smooth Hubble expansion. Using relativistic cosmological perturbation theory, we study the linear evolution of the peculiar velocity field, as well as the expansion/contraction, the shear and the rotation of the bulk motion. Our solutions show growth rates considerably stronger than those of the earlier treatments, which were mostly Newtonian. On scales near and beyond the Hubble radius, namely at the long-wavelength limit, peculiar velocities are found to grow as $$a^2$$a2, in terms of the scale factor, instead of the Newtonian $$a^{1/2}$$a1/2-law. We attribute this to the fact that, in general relativity, the energy flux, triggered here by the peculiar motion of the matter, also contributes to the local gravitational field. In a sense, the bulk flow gravitates, an effect that has been bypassed in related relativistic studies. These stronger growth-rates imply faster peculiar velocities at horizon crossing and higher residual values for the peculiar-velocity field. Alternatively, one could say that our study favours bulk peculiar flows larger and faster than anticipated.

scholarly journals The large-scale distribution of IRAS galaxies and the predicted peculiar velocity field

1991 ◽  
Vol 252 (1) ◽  
pp. 1-12 ◽  
Author(s):  
N. Kaiser ◽  
G. Efstathiou ◽  
R. Ellis ◽  
C. Frenk ◽  
A. Lawrence ◽  
...  
Keyword(s):  
Velocity Field ◽  
Large Scale ◽  
Peculiar Velocity
Sign in / Sign up

Export Citation Format

Share Document