Add to ORKGGalaxy clusters are important targets for peculiar velocity studies as a direct comparison of the various distance indicators can be made. The potential problem of an environmental effect biasing the distances to clusters of different richness is examined. The level of intrinsic cluster-to-cluster variations is also reviewed. We investigate the claim that the derived Fundamental Plane (FP) distances vary systematically with FP scatter. The cluster distances and peculiar velocities derived from Tully-Fisher, FP and Brightest Cluster Galaxies are compared and we find good agreement
As part of an extensive data mining effort, we have compiled a database of 162 Galactic rotation spe...
We derive the relative distances to the Virgo, Fornax and Coma clusters of galaxies by applying the ...
Starting from the observed distribution of Abell/ACO galaxy clusters in redshift space, we use a two...
Galaxy clusters are important targets for peculiar velocity studies as a direct comparison of the va...
We have analyzed the Fundamental Plane (FP) for a sample of 226 E and S0 galaxies in ten clusters of...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
The origin of distance-indicator relations for galaxies is examined, as well as the possibility that...
In this paper we derive a Tully Fisher relation from measured I band photometry and H\alpha rotation...
The distance to the Large Magellanic Cloud (LMC) represents a key local rung of the extragalactic di...
In preceding papers of this series, TF relations for galaxies in 24 clusters with radial velocities ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Velocity dispersion $\sigma$, radius $R$ and luminosity $L$ of elliptical galaxies are known to be r...
We use the Cluster-EAGLE simulations to explore the velocity bias introduced when using galaxies, ra...
6 pages, 1 table, 3 figures, accepted in A&AWe investigate in this paper the error on the cluster re...
The density and velocity fields as extracted from the Abell/ACO clusters are compared to the corresp...
As part of an extensive data mining effort, we have compiled a database of 162 Galactic rotation spe...
We derive the relative distances to the Virgo, Fornax and Coma clusters of galaxies by applying the ...
Starting from the observed distribution of Abell/ACO galaxy clusters in redshift space, we use a two...
Galaxy clusters are important targets for peculiar velocity studies as a direct comparison of the va...
We have analyzed the Fundamental Plane (FP) for a sample of 226 E and S0 galaxies in ten clusters of...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
The origin of distance-indicator relations for galaxies is examined, as well as the possibility that...
In this paper we derive a Tully Fisher relation from measured I band photometry and H\alpha rotation...
The distance to the Large Magellanic Cloud (LMC) represents a key local rung of the extragalactic di...
In preceding papers of this series, TF relations for galaxies in 24 clusters with radial velocities ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Velocity dispersion $\sigma$, radius $R$ and luminosity $L$ of elliptical galaxies are known to be r...
We use the Cluster-EAGLE simulations to explore the velocity bias introduced when using galaxies, ra...
6 pages, 1 table, 3 figures, accepted in A&AWe investigate in this paper the error on the cluster re...
The density and velocity fields as extracted from the Abell/ACO clusters are compared to the corresp...
As part of an extensive data mining effort, we have compiled a database of 162 Galactic rotation spe...
We derive the relative distances to the Virgo, Fornax and Coma clusters of galaxies by applying the ...
Starting from the observed distribution of Abell/ACO galaxy clusters in redshift space, we use a two...