X-ray and radio emission of kiloparsec jets at large redshifts

For some jets of core dominant quasars we assumed that the X-ray emission of the nearest to the core knots is produced by the inverse Compton scattering on the quasar emission whereas the X-ray emission of distant knots is formed by the inverse Compton scattering on the cosmic microwave background a...

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Bibliographic Details
Published in:Advances in Astronomy and Space Physics
Date:2012
Main Author: Mykhailova, M.S.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119152
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:X-ray and radio emission of kiloparsec jets at large redshifts / M.S. Mykhailova // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 49-52. — Бібліогр.: 11 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine