SIMBAD references

2006MNRAS.371...29E - Mon. Not. R. Astron. Soc., 371, 29-37 (2006/September-1)

Extended inverse-Compton emission from distant, powerful radio galaxies.

ERLUND M.C., FABIAN A.C., BLUNDELL K.M., CELOTTI A. and CRAWFORD C.S.

Abstract (from CDS):

We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C432 and 3C191 (z = 1.785 and 1.956, respectively), both of which show extended X-ray emission along the axis of the radio jet or lobe. This X-ray emission is most likely to be due to inverse-Compton scattering of cosmic microwave background (CMB) photons. Under this assumption, we estimate the minimum energy contained in the particles responsible. This can be extrapolated to determine a rough estimate of the total energy. We also present new, deep radio observations of 3C294, which confirm some association between radio and X-ray emission along the north-east-south-west radio axis and also that radio emission is not detected over the rest of the extent of the diffuse X-ray emission. This together with the offset between the peaks of the X-ray and radio emissions may indicate that the jet axis in this source is precessing.

Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS

Journal keyword(s): galaxies: jets - X-rays: individual: 3C191 - X-rays: individual: 3C294 - X-rays: individual: 3C432

Simbad objects: 7

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