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Particular features of γ radiation from active galactic nuclei

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Bulletin of the Crimean Astrophysical Observatory

Abstract

The luminosity of γ radiation from active galactic nuclei is shown to grow with increasing distance to the object. Absorbance of very high-energy γ quanta is far less than the values published so far. High-energy particles are accelerated more effectively when the galactic radiation is enhanced.

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Authors and Affiliations

  1. Crimean Astrophysical Observatory, Nauchnyi, Crimea, 98409, Ukraine

    Yu. I. Neshpor

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  1. Yu. I. Neshpor
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Correspondence to Yu. I. Neshpor.

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Original Russian Text © Yu.I. Neshpor, 2011, published in Izvestiya Krymskoi Astrofizicheskoi Observatorii, 2011, Vol. 107, pp. 38–45.

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Neshpor, Y.I. Particular features of γ radiation from active galactic nuclei. Bull.Crim. Astrophys. Observ. 107, 25–29 (2011). https://doi.org/10.3103/S019027171101013X

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  • DOI: https://doi.org/10.3103/S019027171101013X

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