VLBI observations of 3C273 at 22 GHz and 43 GHz. II: test of Synchrotron Self-Compton process
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The VLBI observations at 22 GHz and 43 GHz of the quasar 3C273 obtained during a multi-frequency campaign in late 1992 in the radio, millimetre and X-ray bands allow us to derive the components' angular sizes, their peak fluxes and turnover frequencies. Lower limits to the Doppler factors have been derived by comparing the observed X-ray fluxes with those predicted by the Synchrotron Self-Compton model. Independent estimates of the Doppler factors were obtained through the assumption of the energy equipartition between the particles and the magnetic field. Of the five components used to model the first two milli-arcseconds of the jet, apart from the core, two components are in equipartition and the remaining two, at larger distances from the core, have large Doppler factors and are mainly responsible for the X-ray emission due to the Synchrotron Self-Compton process.
12 pages, plain tex, plus 2 .ps figures, accepted by Astronomy and Astrophysics, Main Journal, also available at http://www.bo.astro.it/bap/BAPhome/bap99-32-text.ps
12 pages, plain tex, plus 2 .ps figures, accepted by Astronomy and Astrophysics, Main Journal, also available at http://www.bo.astro.it/bap/BAPhome/bap99-32-text.ps