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The Chandra X-ray image of the powerful radio galaxy Cygnus A. The bright
spot in the center is the nucleus of the galaxy, while the two bright spots
to the upper right and the one to the lower left are X-ray emission from the
radio synchrotron hot spots at the outer edges of the radio lobes. The
X-rays from the hot spots result from inverse Compton scattering of the
radio synchrotron radiation by the radio-emitting electrons. The overall
``football-shaped'' structure represents the effect of the radio jets on the
intracluster gas in the cluster of galaxies of which Cygnus A is a member;
the jets inflate a low density bubble and compress the surrounding gas,
which has a temperature of tens of millions K.
Reference: A. S. Wilson, A. J. Young \& P. L. Shopbell,
``Chandra Observations of Cygnus A: Magnetic Field Strengths in the Hot
Spots of a Radio Galaxy'', Astrophys. J. Letters {\bf 544}, L27 (2000)
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