Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

A LARGE-SCALE SHOCK SURROUNDING A POWERFUL RADIO GALAXY?

Journal Article · · Astrophysical Journal Letters
 [1]; ;  [2];  [3];  [4];  [5]
  1. School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ (United Kingdom)
  2. School of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, Hertfordshire, AL10 9AB (United Kingdom)
  3. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)
  4. Department of Physics and Astronomy, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623 (United States)
  5. Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo (Netherlands)
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio galaxy 3C 444. Our 20 ks observation allows us to identify a clear surface brightness drop around the outer edge of the radio galaxy, which is likely to correspond to a spheroidal shock propagating into the intracluster medium. We measure a temperature jump across this drop of a factor {approx}1.7, which corresponds to a Mach number of {approx}1.7. This is likely to be an underestimate due to the need to average over fairly large regions. We also detect clear cavities corresponding to the positions of the radio lobes, which is only the second such detection associated with an FRII radio galaxy. We estimate that the total energy transferred to the environment is >8.2 x 10{sup 60} erg, corresponding to a jet power >2.9 x 10{sup 45} erg s{sup -1}. Our results suggest that energy input from FRII radio galaxies is likely to exceed substantially estimates based on cluster cavity scaling relations.
OSTI ID:
21562596
Journal Information:
Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 2 Vol. 734; ISSN 2041-8205
Country of Publication:
United States
Language:
English

Similar Records

A CHANDRA OBSERVATION OF 3C 288-REHEATING THE COOL CORE OF A 3 keV CLUSTER FROM A NUCLEAR OUTBURST at z = 0.246
Journal Article · Wed Oct 20 00:00:00 EDT 2010 · Astrophysical Journal · OSTI ID:21464596

A POWERFUL AGN OUTBURST IN RBS 797
Journal Article · Tue May 10 00:00:00 EDT 2011 · Astrophysical Journal · OSTI ID:21576889

AN ACTIVE GALACTIC NUCLEUS DRIVEN SHOCK IN THE INTRACLUSTER MEDIUM AROUND THE RADIO GALAXY 3C 310
Journal Article · Tue Apr 10 00:00:00 EDT 2012 · Astrophysical Journal · OSTI ID:22020509