Extragalactic jets on subpc and large scales |
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Authors: | F Tavecchio |
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Institution: | (1) INAF/OAB, via E. Bianchi 46, 23807 Merate (Lc), Italy |
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Abstract: | Jets can be probed in their innermost regions (d≲0.1 pc) through the study of the relativistically boosted emission of blazars. On the other extreme of spatial scales, the study of structure and dynamics of extragalactic relativistic jets received
renewed impulse after the discovery, made by Chandra, of bright X-ray emission from regions at distances larger than hundreds of kpc from the central engine. At both scales it
is thus possible to infer some of the basic parameters of the flow (speed, density, magnetic field intensity, power). After
a brief review of the available observational evidence, I discuss how the comparison between the physical quantities independently
derived at the two scales can be used to shed light on the global dynamics of the jet, from the innermost regions to the hundreds
of kpc scale. |
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Keywords: | Galaxies: active Galaxies: jets (Galaxies:) quasars: X-rays: galaxies |
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