2008/06/10 by P. Rossi, A. Mignone, G. Bodo +2 · 6 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysical jet #Astrophysics and Cosmic Phenomena #BL Lac object #Gamma-ray bursts and supernovae #Jet (fluid) #Lorentz factor #Relativistic beaming #Relativistic particle #Relativistic speed #Superluminal motion #Very-long-baseline interferometry #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809687
20 pages, 17 figures, A&A accepted
arxiv created 2008/06/10 · openalex publication_date 2008/07/17 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Strong observational evidence indicates that all extragalactic jets associated with AGNs move at relativistic speed up to 100 pc-1 kpc scales from the nucleus. At greater distances, reflecting the Fanaroff-Riley radio source classification, we observe an abrupt deceleration in FR-I jets while relativistic motions persist up to Mpc scale in FR-II. Moreover, VLBI observations of some object such as B2 1144+35, Mrk501 and M87 show limb brightening of the jet radio emission on the parsec scale. This effect is interpreted kinematically as due to the deboosted central spine at high Lorentz factor and of a weakly relativistic external layer.