Estimate of the total kinetic power and age of extragalactic jet by its cocoon dynamics: The case of Cygnus A
arXiv:astro-ph/0506626 · doi:10.1111/j.1365-2966.2005.09580.x
Abstract
We examine the constraints imposed on the total kinetic power () and the age () of relativistic jets in FR II radio sources in a new way. We solve the dynamical expansion of its cocoon embedded in the intra-cluster medium (ICM) and obtain the analytic solution of its physical quantities in terms of and . The estimate of and is done by the comparison of the model and the observed shape of the cocoon. The analysis is focused on Cygnus A and we find that (i) the source age is and (ii) the total kinetic power of the jet is estimated as which is larger than 1% of the Eddington luminosity of Cygnus A.
arXiv comment6 pages, 4 figures; MNRAS accepted, final version
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