Skip navigation
Skip navigation

Modeling x-ray emission of a straight jet: PKS 0920-397

Schwartz, D A; Massaro, A; Siemiginowska, A; Worrall, D M; Birkinshaw, M; Marshall, H L; Evans, D; Perlman, E; Gelbord, J; Lovell, J; Godfrey, Leith; Bicknell, Geoffrey; Ojha, R; Hardcastle, M; Jester, S; Jorstad, S; Stawarz, L


We summarize a study of PKS 0920-397 using our 42 ks Chandra observation in conjunction with our ATCA 20GHz image, and HST/ACS F814W and F475W images. We investigate the hypothesis that the jet X-ray emission is due to inverse-Compton (IC) scattering on the cosmic microwave background (CMB) from the same population of relativistic electrons that give rise to the radio emission. To calculate parameters intrinsic to the source, one must finesse the fact that we do not know the true angle of the...[Show more]

CollectionsANU Research Publications
Date published: 2010
Type: Journal article
Source: International Journal of Modern Physics D:
DOI: 10.1142/S0218271810017147


File Description SizeFormat Image
01_Schwartz_Modeling_x-ray_emission_of_a_2010.pdf299.87 kBAdobe PDFThumbnail

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  19 May 2020/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator