Abstract
It is shown that composite radio spectra of the hot spots of the radio galaxy Cygnus A can be fully explained by assuming a nonuniform distribution of the magnetic fields inside the hot spots, without invoking any physical mechanisms other than synchrotron radiation. The magnetic fields are strong (B ∼ 10−2−10−1 G) at the center of the hot spots, and decreases at the hot-spot edges to the level of the magnetic field of the radio lobes in which the hot spots are embedded (B ∼ 10−4−10−5 G). The difference in the magnetic field between the hot-spot center and edge decreases during the evolution, while the average magnetic-field intensity increases.
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Original Russian Text © V.S. Artyukh, S.A. Tyul’bashev, P.A. Chernikov, 2012, published in Astronomicheskii Zhurnal, 2012, Vol. 89, No. 9, pp. 754–760.
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Artyukh, V.S., Tyul’bashev, S.A. & Chernikov, P.A. Physical conditions in the hot spots of the radio galaxy Cygnus A. Astron. Rep. 56, 680–685 (2012). https://doi.org/10.1134/S1063772912090016
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DOI: https://doi.org/10.1134/S1063772912090016