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A Large-scale Shock Surrounding a Powerful Radio Galaxy?

  • Authors: J. H. Croston, M. J. Hardcastle, B. Mingo, D. A. Evans, D. Dicken, R. Morganti, and C. N. Tadhunter

Croston et al. 2011 The Astrophysical Journal Letters 734 L28.

  • Provider: AAS Journals

Caption: Figure 4.

X-ray surface brightness profiles of the emission surrounding 3C 444. The emission was divided into four quadrants, with the north and south quadrants combined to make a longitudinal profile (black) and the east and west quadrants combined to make a transverse profile (red). A sharp drop is present in the N–S direction at ~45 arcsec, while a less sharp drop is present at ~30 arcsec in the E–W direction.

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