A Possibile Dichotomy Between PC Scale Jets of Brightest Cluster Galaxies in Cool Core and Non-Cool Core Clusters

Details A Possibile Dichotomy Between PC Scale Jets of Brightest Cluster Galaxies in Cool Core and Non-Cool Core Clusters A Possibile Dichotomy Between PC Scale Jets of Brightest Cluster Galaxies in Cool Core and Non-Cool Core Clusters

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..427..351l&link_type=abstract

Accretion and Ejection in AGN: a Global View. Proceedings of a conference held June 22-26, 2009 in Como, Italy. Edited by Laura

Physics

Scientific paper

We present a statistical study on parsec scale properties of a sample of Brigthest Cluster Galaxies (BCGs) in 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 the two-sided morphology in cool core clusters could be due to the presence of mildly relativistic jets slowed down already at mas scale as consequence of the jet interaction with a dense surrounding medium.

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