Blazars and the emerging AGN/black hole X-ray binary paradigm

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dc.creatorUttley, P.
dc.date2005-08-02
dc.date.accessioned2026-07-07T02:18:22Z
dc.date.available2026-07-07T02:18:22Z
dc.descriptionWe briefly review the emerging paradigm which links the radio-quiet and radio-loud classes of AGN to the different accretion states observed in stellar mass black hole X-ray binary systems (BHXRBs), and discuss the relevance of the AGN/BHXRB connection to blazar variability.
dc.description4 pages, 1 figure, to appear in the proceedings of the workshop on `Blazar Variability: entering the GLAST Era', Miami, April 2005 (ASP Conf. Series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0508060
dc.identifierhttp://arxiv.org/abs/astro-ph/0508060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9464
dc.subjectAstrophysics
dc.titleBlazars and the emerging AGN/black hole X-ray binary paradigm
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