Extended inverse-Compton emission from distant, powerful radio galaxies
We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=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...
Main Authors: | , , , , |
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Formato: | Journal article |
Idioma: | English |
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2006
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author | Erlund, M Fabian, A Blundell, K Celotti, A Crawford, C |
author_facet | Erlund, M Fabian, A Blundell, K Celotti, A Crawford, C |
author_sort | Erlund, M |
collection | OXFORD |
description | We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=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 3C 294, which confirm some association between radio and X-ray emission along the NE-SW 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. |
first_indexed | 2024-03-07T00:54:29Z |
format | Journal article |
id | oxford-uuid:878d745c-16f5-4ee6-8fca-8fe29389ed40 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T00:54:29Z |
publishDate | 2006 |
record_format | dspace |
spelling | oxford-uuid:878d745c-16f5-4ee6-8fca-8fe29389ed402022-03-26T22:11:28ZExtended inverse-Compton emission from distant, powerful radio galaxiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:878d745c-16f5-4ee6-8fca-8fe29389ed40EnglishSymplectic Elements at Oxford2006Erlund, MFabian, ABlundell, KCelotti, ACrawford, CWe present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=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 3C 294, which confirm some association between radio and X-ray emission along the NE-SW 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. |
spellingShingle | Erlund, M Fabian, A Blundell, K Celotti, A Crawford, C Extended inverse-Compton emission from distant, powerful radio galaxies |
title | Extended inverse-Compton emission from distant, powerful radio galaxies |
title_full | Extended inverse-Compton emission from distant, powerful radio galaxies |
title_fullStr | Extended inverse-Compton emission from distant, powerful radio galaxies |
title_full_unstemmed | Extended inverse-Compton emission from distant, powerful radio galaxies |
title_short | Extended inverse-Compton emission from distant, powerful radio galaxies |
title_sort | extended inverse compton emission from distant powerful radio galaxies |
work_keys_str_mv | AT erlundm extendedinversecomptonemissionfromdistantpowerfulradiogalaxies AT fabiana extendedinversecomptonemissionfromdistantpowerfulradiogalaxies AT blundellk extendedinversecomptonemissionfromdistantpowerfulradiogalaxies AT celottia extendedinversecomptonemissionfromdistantpowerfulradiogalaxies AT crawfordc extendedinversecomptonemissionfromdistantpowerfulradiogalaxies |