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20 April 2024
 
  » arxiv » astro-ph/0008442

 Article overview


VSOP observation of the quasar PKS 2215+020: a new laboratory for core-jet physics at z=3.572
A.P. Lobanov ; L.I. Gurvits ; S. Frey ; R.T. Schilizzi ; K.I. Kellermann ; N. Kawaguchi ; I.I.K. Pauliny-Toth ;
Date 29 Aug 2000
Subject astro-ph
AbstractWe report results of a VSOP (VLBI Space Observatory Programme) observation of a high redshift quasar PKS 2215+020 (z=3.572). The ~1 milliarcsecond resolution image of the quasar reveals a prominent `core-jet’ structure on linear scales from 5/h to 300/h pc ($H_0=100*h km/(s*Mpc). The brightness temperatures and sizes of bright features identified in the jet are consistent with emission from relativistic shocks dominated by adiabatic energy losses. The jet is powered by the central black hole with estimated mass of ~4*10^9 solar masses. Comparisons with VLA and ROSAT observations indicate a possible presence of an extended radio/X-ray halo surrounding 2215+020.
Source arXiv, astro-ph/0008442
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