Volume 422, Number 2, August I 2004
|Page(s)||515 - 522|
|Published online||09 July 2004|
Radio galaxies in cooling core clusters. Renewed activity in the nucleus of 3C 317?
Istituto di Radioastronomia del CNR, via Gobetti 101, 4129 Bologna, Italy e-mail: firstname.lastname@example.org
2 Dipartimento di Astronomia, via Ranzani 1, 40127 Bologna, Italy
Accepted: 27 April 2004
We present the results of VLBA observations of the radio galaxy 3C 317, associated with the cD galaxy UGC 09799 at the centre of the cooling core cluster of galaxies A2052. These observations were carried out at 1.7 GHz, 4.9 GHz and 8.3 GHz, in polarimetric mode, and allowed us to image the parsec scale region of the source. Our analysis suggests that the nucleus of 3C 317 hosts a very young radio source. The estimated radiative age for the radio structure within the inner 10 pc is ~170 yr. Given the existence of extended radio emission on the arcsecond scale, we suggest that 3C 317 is a restarted radio galaxy. The implications of this result in the light of the interaction between radio plasma and thermal hot gas in clusters of galaxies are briefly discussed.
Key words: galaxies: clusters: individual: Abell 2052 / galaxies: structure / radio continuum: galaxies
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.