Anisotropic inverse Compton scattering in radio galaxies and particle energy distribution

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dc.creatorBrunetti, G.
dc.creatorSetti, G.
dc.date2000-10-31
dc.date.accessioned2026-07-07T01:56:19Z
dc.date.available2026-07-07T01:56:19Z
dc.descriptionIn this talk we briefly review the inverse Compton (IC) scattering of nuclear photons in the lobes of radio galaxies and quasars. We concentrate on the possibility to test this model with the Chandra observatory and to constrain the electron energy distribution by measuring the X-ray fluxes produced by this effect. We also discuss the evidence for IC scattering of nuclear photons in the powerful radio galaxies.
dc.description4 pages, 4 .ps figure, uses newpaspsty (included). To appear in "Particles and Fields in Radio Galaxies", R.A.Laing and K.M.Blundell (Eds.), to be published by the Astronomical Society of the Pacific (ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0010651
dc.identifierhttp://arxiv.org/abs/astro-ph/0010651
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1957
dc.subjectAstrophysics
dc.titleAnisotropic inverse Compton scattering in radio galaxies and particle energy distribution
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