Parsec Scale Properties of Brightest Cluster Galaxies
| dc.creator | Giovannini, G. | |
| dc.creator | Liuzzo, E. | |
| dc.creator | Giroletti, M. | |
| dc.date | 2008-02-25 | |
| dc.date.accessioned | 2026-07-07T09:22:59Z | |
| dc.date.available | 2026-07-07T09:22:59Z | |
| dc.description | We present new VLBI observations of Brightest Cluster Galaxies in eight nearby Abell clusters. These data show a possible difference between Brightest Cluster Galaxies in cool core clusters (two-sided pc scale jets) and in non cool core clusters (one-sided pc scale jets). We suggest that this difference could be due to the jet interaction with the surrounding medium. More data are necessary to discuss if pc-scale properties of Brightest Cluster Galaxies are influenced by their peculiar morphology and position in the center of rich clusters of galaxies. | |
| dc.description | 4 pages. Contributed talk. To be published in the proceedings of: "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology". Eds. Y. Hagiwara, E. Fomalont, M. Tsuboi, and Y. Murata | |
| dc.identifier | https://arxiv.org/abs/0802.3574 | |
| dc.identifier | http://arxiv.org/abs/0802.3574 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/155574 | |
| dc.subject | Astrophysics | |
| dc.title | Parsec Scale Properties of Brightest Cluster Galaxies | |
| dc.type | text |