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Kiloparsec-Scale Jets in FR I Radio Galaxies and the Gamma-Ray Background

L. Stawarz·T. M. Kneiske·J. Kataoka
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Abstract

We discuss the contribution of kiloparsec-scale jets in FR I radio galaxies to the diffuse gamma-ray background radiation. The analyzed gamma-ray emission comes from inverse-Compton scattering of starlight photon fields by the ultrarelativistic electrons whose synchrotron radiation is detected from such sources at radio, optical and X-ray energies. We find that these objects, under the minimum-power hypothesis (corresponding to a magnetic field of 300 muG in the brightest knots of these jets), can contribute about one percent to the extragalactic gamma-ray background measured by EGRET. We point out that this result already indicates that the magnetic fields in kpc-scale jets of low-power radio galaxies are not likely to be smaller than 10 muG on average, as otherwise the extragalactic gamma-ray background would be overproduced.

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L. Stawarz, T. M. Kneiske, J. Kataoka. 2005-09-14. Kiloparsec-Scale Jets in FR I Radio Galaxies and the Gamma-Ray Background. https://doi.org/10.1086/498084

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