期刊
ASTROPHYSICAL JOURNAL
卷 580, 期 1, 页码 110-113出版社
IOP PUBLISHING LTD
DOI: 10.1086/343112
关键词
galaxies : active; galaxies : individual (M84); galaxies : jets; radiation mechanisms : nonthermal; radio continuum : galaxies; X-rays : galaxies
During the course of an investigation of the interaction of the radio galaxy M84 and its ambient cluster gas, we found excess X-ray emission aligned with the northern radio jet. The emission extends from the X-ray core of the host galaxy as a weak bridge and then brightens to a local peak coincident with the first detectable radio knot at approximate to2.5 from the core. The second radio knot at 3.3 is brighter in both radio and X-ray. The X-ray jet terminates 3.9 from the core. Although all the evidence suggests that Doppler favoritism augments the emission of the northern jet, it is unlikely that the excess X-ray emission is produced by inverse Compton emission. We find many similarities between the M84 X-ray jet and recent jet detections from Chandra data of low-luminosity radio galaxies. For most of these current detections, synchrotron emission is the favored explanation for the observed X-rays.
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