Extended inverse compton emission from distant powerful radio galaxies
Chandra observations of 3C432, 3C 191 and B2 0902+34 are presented as part of an ongoing search for inverse-Compton scattering of the cosmic microwave background (CMB) from high redshift radio sources (Schwartz, 2000). The energy density of the CMB increases with redshift, z, as (1 + z)4, so the rel...
Päätekijät: | Erlund, M, Fabian, A, Blundell, K, Celotti, A, Crawford, C |
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Aineistotyyppi: | Journal article |
Kieli: | English |
Julkaistu: |
2006
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