Abstract
Chandra X-ray Observatory observations of the powerful, peculiar radio galaxy 3C 123 have resulted in an X-ray detection of the bright eastern hot-spot, with a 1-ke V flux density of ~5 nJy. The X-ray flux and spectrum of the hot-spot are consistent with the X-rays being inverse-Compton emission from the population of electrons responsible for the radio emission, if the magnetic fields in the hot-spot are close to their equipartition values. 3C 123 is thus the third radio galaxy to show direct evidence for equipartition in hot-spots.
Original language | English |
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Title of host publication | In: Procs of Particles and Fields in Radio Galaxies Conference, ASP Conference Proceedings 250 |
Publisher | Astronomical Society of the Pacific |
Pages | 234-237 |
ISBN (Print) | 1-58381-090-0 |
Publication status | Published - 2001 |