Probing the physics of relativistic jets through X-ray observations

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dc.creatorMaraschi, L.
dc.creatorTavecchio, F.
dc.date2001-07-30
dc.date.accessioned2026-07-07T01:59:28Z
dc.date.available2026-07-07T01:59:28Z
dc.descriptionThe broad band sensitivity and flexibility of the BeppoSAX satellite have allowed unprecedented studies of the X-ray emission from blazars. Here we focus on recent results on the SEDs of a group of blazars with emission lines, allowing to estimate both the luminosity in the jet and the luminosity of the accretion disk. Implications for the origin of the power carried by relativistic jets are considered.
dc.description9 pages, 4 figures, presented at "X-ray Astronomy 2000" meeting, Palermo, Italy, Sept. 2000. Proceedings to be published in ASP Conference series, eds. R. Giacconi, L. Stella, & S. Serio, 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0107566
dc.identifierhttp://arxiv.org/abs/astro-ph/0107566
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3130
dc.subjectAstrophysics
dc.titleProbing the physics of relativistic jets through X-ray observations
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