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Ruling out IC/CMB X-Rays in PKS 0637-752 and the implications for TEV emission from large-scale quasar jets


Meyer, ET and Georganopoulos, M and Sparks, WB and Godfrey, L and Lovell, JEJ and Perlman, E, Ruling out IC/CMB X-Rays in PKS 0637-752 and the implications for TEV emission from large-scale quasar jets, Astrophysical Journal, 805, (2) Article 154. ISSN 0004-637X (2015) [Refereed Article]


Copyright Statement

2015. The American Astronomical Society. All rights reserved.

DOI: doi:10.1088/0004-637X/805/2/154


The Chandra X-ray observatory has discovered dozens of resolved, kiloparsec-scale jets associated with powerful quasars in which the X-ray fluxes are observed to be much higher than the expected level based on the radio-optical synchrotron spectrum. The most popular explanation for the anomalously high and hard X-ray fluxes is that these jets do not decelerate significantly by the kiloparsec scale, but rather remain highly relativistic (Lorentz factors Γ ~ 10). By adopting a small angle to the line of sight, the X-rays can thus be explained by inverse Compton upscattering of cosmic microwave background (CMB) photons (IC/CMB), where the observed emission is strongly Doppler boosted. Using over six years of Fermi monitoring data, we show that the expected hard, steady gamma-ray emission implied by the IC/CMB model is not seen in PKS 0637-752, the prototype jet for which this model was first proposed. IC/CMB emission is thus ruled out as the source of the X-rays, joining recent results for the jets in 3C 273 (using the same method) and PKS 1136-135 (using UV polarization). We further show that the Fermi observations give an upper limit of δ < 6.5 for the four brightest X-ray knots of PKS 0637-752, and derive an updated limit of δ < 7.8 for knots A and B1 of 3C 273 (assuming equipartition). Finally, we discuss the fact that high levels of synchrotron X-ray emission in a slow jet will unavoidably lead to a level of angle-integrated TeV emission which exceeds that of the TeV BL Lac class.

Item Details

Item Type:Refereed Article
Keywords:galaxies: active, galaxies: jets, quasars: individual: PKS 0637-752, 3C 273
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Cosmology and extragalactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Lovell, JEJ (Dr Jim Lovell)
ID Code:105943
Year Published:2015
Web of Science® Times Cited:61
Deposited By:Mathematics and Physics
Deposited On:2016-01-20
Last Modified:2017-11-03
Downloads:190 View Download Statistics

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