Evidence for a low-density universe from the relative velocities of galaxies

Evidence for a low-density universe from the relative velocities of galaxies

Mostrar outras versões (1)

The motions of galaxies can be used to constrain the cosmological density parameter Omega and the clustering amplitude of matter on large scales. The mean relative velocity of galaxy pairs, estimated from the Mark III survey, indicates that Omega = 0.35(-0.25)(+0.35). If the clustering of galaxies i...

ver descrição completa

Detalhes bibliográficos
Principais autores:	Juszkiewicz, R, Ferreira, P, Feldman, H, Jaffe, A, Davis, M
Formato:	Journal article
Idioma:	English
Publicado em:	2000

Registros relacionados

Evidence for a low-density Universe from the relative velocities of galaxies
por: Juszkiewicz, R, et al.
Publicado em: (2000)

Measuring Ω with Galaxy Streaming Velocities
por: Ferreira, P, et al.
Publicado em: (1999)

Streaming velocities as a dynamical estimator of Omega
por: Ferreira, P, et al.
Publicado em: (1998)

Streaming velocities as a dynamical estimator of Omega
por: Ferreira, P, et al.
Publicado em: (1999)

Power Spectrum Estimation from Peculiar Velocity Catalogues
por: Macaulay, E, et al.
Publicado em: (2011)

Power spectrum estimation from peculiar velocity catalogues
por: MacAulay, E, et al.
Publicado em: (2012)

Linear relation between H i circular velocity and stellar velocity dispersion in early-type galaxies, and slope of the density profiles
por: Serra, P, et al.
Publicado em: (2016)

The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe
por: Hawkins, E, et al.
Publicado em: (2003)

The relation between gas density and velocity power spectra in galaxy clusters: qualitative treatment and cosmological simulations
por: Zhuravleva, I, et al.
Publicado em: (2014)

Line-of-sight velocity distributions of low-luminosity elliptical galaxies
por: Halliday, C, et al.
Publicado em: (2001)

Early-type galaxies in low-density environments
por: Kuntschner, H, et al.
Publicado em: (2002)

THE RELATIVE AMPLITUDES OF MANTLE HETEROGENEITY IN P-VELOCITY, S-VELOCITY AND DENSITY FROM FREE-OSCILLATION DATA
por: Li, X, et al.
Publicado em: (1991)

Age velocity dispersion relations and heating histories in disc galaxies
por: Aumer, M, et al.
Publicado em: (2016)

A Slight Excess of Large Scale Power from Moments of the Peculiar Velocity Field
por: Macaulay, E, et al.
Publicado em: (2010)

The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe
por: Verde, L, et al.
Publicado em: (2002)

The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
por: Verde, L, et al.
Publicado em: (2002)

The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum
por: Lelli, F, et al.
Publicado em: (2019)

Central stellar populations of early-type galaxies in low-density environments
por: Collobert, M, et al.
Publicado em: (2006)

Determination of Shear Wave Velocity and Attenuation From Waveforms in Low Velocity Formations
por: Toksoz, M. Nafi, et al.
Publicado em: (2012)

ELLIPTIC GALAXIES AND LARGE-SCALE VELOCITY FLOWS
por: Faber, S, et al.
Publicado em: (1988)

RADIUS-DEPENDENCE OF VELOCITY DISPERSION IN ELLIPTICAL GALAXIES
por: Binney, J
Publicado em: (1980)

On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
por: Han, S, et al.
Publicado em: (2024)

Galaxy ecology : groups and low-density environments in the SDSS and 2dFGRS
por: Balogh, M, et al.
Publicado em: (2004)

Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS
por: Balogh, M, et al.
Publicado em: (2004)

Simultaneous inversion of velocity and density profiles
Publicado em: (2003)

THE METALLICITIES, VELOCITY DISPERSIONS AND TRUE SHAPES OF ELLIPTICAL GALAXIES
por: Terlevich, R, et al.
Publicado em: (1981)

The velocity and mass distribution of clusters of galaxies from the CNOC1 cluster redshift survey
por: van der Marel, R, et al.
Publicado em: (2000)

The SAMI Galaxy Survey: Mass as the driver of the kinematic morphology-density relation in clusters
por: Brough, S, et al.
Publicado em: (2017)

An estimate of Ω_m without priors
por: Feldman, H, et al.
Publicado em: (2003)

ELECTRON-DENSITIES IN ACTIVE GALAXIES
por: Jordan, C
Publicado em: (1983)

Uncorrelated velocity and size residuals across galaxy rotation curves
por: Desmond, H, et al.
Publicado em: (2019)

The tight empirical relation between dark matter halo mass and flat rotation velocity for late-type galaxies
por: Katz, H, et al.
Publicado em: (2018)

PREDICTING LINE-OF-SIGHT VELOCITY DISTRIBUTIONS OF ELLIPTIC GALAXIES
por: Magorrian, J, et al.
Publicado em: (1994)

Position-velocity diagrams in the inner regions of disk galaxies
por: Funes, J, et al.
Publicado em: (2001)

HIGH-VELOCITY CLOUDS IN THE NEARBY SPIRAL GALAXY M 83
por: Bregman, Joel N., et al.
Publicado em: (2015)

An estimate of Omega(m) without conventional priors
por: Feldman, H, et al.
Publicado em: (2003)

OPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY
por: Bautz, Marshall W., et al.
Publicado em: (2015)

ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments
por: Muzzin, A., et al.
Publicado em: (2018)

SPIRAL GALAXIES, ELLIPTIC GALAXIES AND THE LARGE-SCALE VELOCITY-FIELD WITHIN 3500 KM/S OF THE LOCAL GROUP
por: Burstein, D, et al.
Publicado em: (1988)

Evidence for the rapid formation of low-mass early-type galaxies in dense environments
por: Liu, Y, et al.
Publicado em: (2016)