Galaxy 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...
The relationship first pointed out by Tully and Fisher between the luminosity of spiral galaxies and...
Context. The angular diameter distances toward galaxy clusters can be determined with measurements o...
Galaxy clusters are important targets for peculiar velocity studies as a direct comparison of the va...
The origin of distance-indicator relations for galaxies is examined, as well as the possibility that...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
Moriond08The Tully-Fisher relation is a correlation between the luminosity and the HI 21cm line widt...
The peculiar velocity function of clusters of galaxies is determined using an accurate sample of clu...
We derive the relative distances to the Virgo, Fornax and Coma clusters of galaxies by applying the ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
International audienceWe define here a standard candle to determine the distance of clusters of gala...
We have analyzed the Fundamental Plane (FP) for a sample of 226 E and S0 galaxies in ten clusters of...
The distance to the Large Magellanic Cloud (LMC) represents a key local rung of the extragalactic di...
International audienceWe present a new method of bias correction for deriving reliable Tully-Fisher ...
6 pages, 1 table, 3 figures, accepted in A&AWe investigate in this paper the error on the cluster re...
As part of an extensive data mining effort, we have compiled a database of 162 Galactic rotation spe...
The relationship first pointed out by Tully and Fisher between the luminosity of spiral galaxies and...
Context. The angular diameter distances toward galaxy clusters can be determined with measurements o...
Galaxy clusters are important targets for peculiar velocity studies as a direct comparison of the va...
The origin of distance-indicator relations for galaxies is examined, as well as the possibility that...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
Moriond08The Tully-Fisher relation is a correlation between the luminosity and the HI 21cm line widt...
The peculiar velocity function of clusters of galaxies is determined using an accurate sample of clu...
We derive the relative distances to the Virgo, Fornax and Coma clusters of galaxies by applying the ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
International audienceWe define here a standard candle to determine the distance of clusters of gala...
We have analyzed the Fundamental Plane (FP) for a sample of 226 E and S0 galaxies in ten clusters of...
The distance to the Large Magellanic Cloud (LMC) represents a key local rung of the extragalactic di...
International audienceWe present a new method of bias correction for deriving reliable Tully-Fisher ...
6 pages, 1 table, 3 figures, accepted in A&AWe investigate in this paper the error on the cluster re...
As part of an extensive data mining effort, we have compiled a database of 162 Galactic rotation spe...
The relationship first pointed out by Tully and Fisher between the luminosity of spiral galaxies and...
Context. The angular diameter distances toward galaxy clusters can be determined with measurements o...