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most citedThe origin of HI-deficiency in galaxies on the outskirts of the Virgo cluster. I. How far can galaxies bounce out of clusters?

77 citations · 82 across the 4 of their papers we have counts for

collaborators

19 papers

astro-ph2004

DENIS detections of highly obscured galaxies in the area around PKS1343-601

Anja C. Schroeder, Renee C. Kraan-Korteweg, Gary A. Mamon +1

We present results of a search for galaxies around the highly obscured giant radio galaxy PKS1343-601 using the near-infrared DENIS survey. We compare our findings with surveys in…

astro-ph20044 cited

Breaking the mass / anisotropy degeneracy in the Coma cluster

Gary A. Mamon, Ewa L. Lokas, Teresa Sanchis

We provide the first direct lifting of the mass/anisotropy degeneracy for a cluster of galaxies, by jointly fitting the line of sight velocity dispersion and kurtosis profiles of t…

astro-ph200377 cited

The origin of HI-deficiency in galaxies on the outskirts of the Virgo cluster. I. How far can galaxies bounce out of clusters?

G. A. Mamon, T. Sanchis, E. Salvador-Sole' +2

Spiral galaxies that are deficient in neutral Hydrogen are observed on the outskirts of the Virgo cluster. If their orbits have crossed the inner parts of the cluster, their inters…

astro-ph20021 cited

Constraints on dark energy and quintessence with a comoving standard ruler applied to 2dF quasars

Gary A. Mamon, Boud F. Roukema

Structures on very large scales (> 100 Mpc) have negligible peculiar motions, and are thus roughly fixed in comoving space. We looked for significant peaks at very large separation…

astro-ph2001

Where the Very Bright Matter is a Standard Ruler

B. F. Roukema, G. A. Mamon, S. Bajtlik

Where's the matter? The answer seems to be: ``distributed according to a power spectrum with at least one feature (local maximum) near 120-130h^-1Mpc''. Analyses of the Iovino, Clo…

astro-ph1999

Theory of galaxy dynamics in clusters and groups

Gary A. Mamon

Analytical estimates of the mass and radial dependence of the rates of galaxy mergers and of tidal interactions are derived for clusters and groups of galaxies, taking into account…