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- W1533753531 abstract "We discuss the contribution of kiloparsec‐scale jets in FR I radio galaxies to the diffuse γ‐ray background radiation. The analyzed γ‐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 μG in the brightest knots of these jets), can contribute about one percent to the extragalactic γ‐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 μG on average, as otherwise the extragalactic γ‐ray background would be overproduced." @default.
- W1533753531 created "2016-06-24" @default.
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- W1533753531 date "2007-01-01" @default.
- W1533753531 modified "2023-09-23" @default.
- W1533753531 title "Direct and reprocessed γ-ray emission of kpc-scale jets in FR I radio galaxies" @default.
- W1533753531 doi "https://doi.org/10.1063/1.2757353" @default.
- W1533753531 hasPublicationYear "2007" @default.
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