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Parsec Scale Properties of Brightest Cluster Galaxies.

Name: Parsec Scale Properties of Brightest Cluster Galaxies.
Keywords: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 13 Jul 2009Embargo end date: 01 Jan 2009Publisher:Sissa MedialabJournal:Proceedings of The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting — PoS(IX EVN Symposium)

Authors: Gabriele Giovannini; Marcello Giroletti; Elisabetta Liuzzo;

doi: 10.22323/1.072.0017 , 10.48550/arxiv.0903.0812 , 10.48550/arxiv.0802.3574

arXiv: http://arxiv.org/abs/0903.0812 , http://arxiv.org/abs/0802.3574

Parsec Scale Properties of Brightest Cluster Galaxies.

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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.

6 pages, 2 figures. Contributed talk. To be published in the proceedings of "The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting", September 23-26, 2008, Bologna, Italy

Keywords

Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics

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