Spitzer Observations of Centaurus A: Infrared Synchrotron Emission from the Northern Lobe
arXiv:astro-ph/0601413 · doi:10.1086/506472
Abstract
We present measurements obtained with the Spitzer Space Telescope in five bands from 3.6-24 microns of the northern inner radio lobe of Centaurus A, the nearest powerful radio galaxy. We show that this emission is synchrotron in origin. Comparison with ultraviolet observations from GALEX shows that diffuse ultraviolet emission exists in a smaller region than the infrared but also coincides with the radio jet. We discuss the possibility, that synchrotron emission is responsible for the ultraviolet emission and conclude that further data are required to confirm this.
arXiv comment4 pages, accepted by ApJL
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- The -ray spectrum of the core of Centaurus A as observed with H.E.S.S. and Fermi-LAT
- LABOCA observations of nearby, active galaxies
- A Chandra Study of the Lobe/ISM Interactions Around the Inner Radio Lobes of Centaurus A: Constraints on the Temperature Structure and Transport Processes
- Ultra-High Energy Cosmic-Ray Acceleration in the Jet of Centaurus A
- An Infrared Study of the Large-scale Jet in Quasar PKS 1136-135
- The Infrared Jet in 3C31
- Physical conditions in nearby active galaxies correlated with ultra-high-energy cosmic rays detected by the Pierre Auger Observatory
- Optical Detection of Star Formation in a Cold Dust Cloud in the Counterjet Direction of Centaurus A