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Fueling Lobes of Radio Galaxies: Statistical Particle Acceleration and the Extragalactic γ-ray Background

  • Authors: F. Massaro and M. Ajello

Massaro & Ajello 2011 The Astrophysical Journal Letters 729 L12.

  • Provider: AAS Journals

Caption: Figure 1.

(a) B/ B CMB ratio (upper panel) for the FR IIs’ lobes in the sample of C05. The dashed red line indicates the case B/ B CMB = 1, when synchrotron and IC/CMB losses have the same relevance. (b) The equivalent spherical radius of the lobe volume, R lobe, as a function of redshift estimated for the same sample.

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