arXiv · 0903.0812
Parsec Scale Properties of Brightest Cluster Galaxies
Abstract
We present new VLBI observations of a complete sample of Brigthest Cluster Galaxies (BCGs) in nearby Abell Clusters. These data show a possible difference between BCGs in cool core clusters (two-sided parsec scale jets) and in non cool core clusters (one-sided parsec scale jet). We suggest that this difference could be due to the jet interaction with the surrounding medium. More data are necessary to discuss whether parsec-scale properties of BCGs are influenced by their peculiar morphology and position at the center of rich galaxy clusters.
Explore related subjects
Keep this discovery
E. Liuzzo, G. Giovannini, M. Giroletti. 2009-03-04. Parsec Scale Properties of Brightest Cluster Galaxies. https://arxiv.org/abs/0903.0812
Cite the original work for its findings. Save a collection to share your selection of sources.