Redshift Survey Compact Groups (RSCGs) are tight knots of N >= 3 galaxies selected from the CfA2+SSRS2 redshift survey. The selection is based on physical extent and association in redshift space alone. We measured 300 new redshifts of fainter galaxies within 1 h^{-1} Mpc of 14 RSCGs to explore the relationship between RSCGs and their environments. 13 of 14 RSCGs are embedded in overdense regions of redshift space. The systems range from a loose group of 5 members to an Abell cluster. The remaining group, RSCG 64, appears isolated. RSCGs are isolated and distinct from their surroundings to varying degrees, as are the Hickson Compact Groups. Among the 13 embedded RSCGs, 3 are distinct from their general environments (RSCG 9, RSCG 11 and RSCG...
We investigate the properties of photometrically-selected compact groups (CGs) in the Sloan Digital ...
We present the results of a redshift survey of 138 candidate compact groups from the DPOSS II catalo...
Compact groups, with their high number densities, small velocity dispersions, and an interstellar me...
For the first time, we construct a catalog of compact groups selected from a complete, magnitude-lim...
Aims. In this work we present an algorithm to identify compact groups (CGs) that closely follows Hic...
Compact groups are small, relatively isolated, systems of galaxies with projected separations compar...
We use the Sloan Digital Sky Survey (SDSS) redshift catalogue to look for galaxies with accordant re...
In this work we present an algorithm to identify compact groups (CGs) that closely follows Hickson's...
This paper presents the results of a pilot redshift survey of 18 candidate compact groups from the d...
We present the results of a redshift survey of 138 candidate compact groups from the DPOSS II catalo...
Using new data and an enlarged group sample we verify some of our previously published results and p...
Aims. The purpose of this work is to perform a statistical analysis of the location of compact group...
International audienceMany catalogues of isolated compact groups of galaxies (CGs) have been extract...
We investigate the properties of photometrically selected compact groups (CGs) in the Sloan Digital ...
We have systematically analyzed a sample of 13 new and archival ROSAT Position Sensitive Proportiona...
We investigate the properties of photometrically-selected compact groups (CGs) in the Sloan Digital ...
We present the results of a redshift survey of 138 candidate compact groups from the DPOSS II catalo...
Compact groups, with their high number densities, small velocity dispersions, and an interstellar me...
For the first time, we construct a catalog of compact groups selected from a complete, magnitude-lim...
Aims. In this work we present an algorithm to identify compact groups (CGs) that closely follows Hic...
Compact groups are small, relatively isolated, systems of galaxies with projected separations compar...
We use the Sloan Digital Sky Survey (SDSS) redshift catalogue to look for galaxies with accordant re...
In this work we present an algorithm to identify compact groups (CGs) that closely follows Hickson's...
This paper presents the results of a pilot redshift survey of 18 candidate compact groups from the d...
We present the results of a redshift survey of 138 candidate compact groups from the DPOSS II catalo...
Using new data and an enlarged group sample we verify some of our previously published results and p...
Aims. The purpose of this work is to perform a statistical analysis of the location of compact group...
International audienceMany catalogues of isolated compact groups of galaxies (CGs) have been extract...
We investigate the properties of photometrically selected compact groups (CGs) in the Sloan Digital ...
We have systematically analyzed a sample of 13 new and archival ROSAT Position Sensitive Proportiona...
We investigate the properties of photometrically-selected compact groups (CGs) in the Sloan Digital ...
We present the results of a redshift survey of 138 candidate compact groups from the DPOSS II catalo...
Compact groups, with their high number densities, small velocity dispersions, and an interstellar me...