On magnetic fields in broad-line blazars

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dc.creatorModerski, R.
dc.creatorSikora, M.
dc.date2006-12-13
dc.date.accessioned2026-07-07T07:31:08Z
dc.date.available2026-07-07T07:31:08Z
dc.descriptionHigh energy spectra of broad-line blazars can be reproduced by both synchrotron-self-Compton (SSC) models and external-Compton (EC) models. However, as is known from numerical modeling, SSC scenarios require much weaker magnetic field than EC ones. In this paper we quantify these results analytically.
dc.description4 pages, no figures. Conference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP) - unabridged version
dc.identifierhttps://arxiv.org/abs/astro-ph/0612342
dc.identifierhttp://arxiv.org/abs/astro-ph/0612342
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118646
dc.subjectAstrophysics
dc.titleOn magnetic fields in broad-line blazars
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