Radio to X-ray Study of a Sample of 3CRR Sources: Jet Kinetic and Accretion Power

Details Radio to X-ray Study of a Sample of 3CRR Sources: Jet Kinetic and Accretion Power Radio to X-ray Study of a Sample of 3CRR Sources: Jet Kinetic and Accretion Power

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..427..195g&link_type=abstract

Accretion and Ejection in AGN: a Global View. Proceedings of a conference held June 22-26, 2009 in Como, Italy. Edited by Laura

Computer Science

Scientific paper

We performed a study of 93 radio sources belonging to the same 3CRR sample but characterized by different radio and optical classifications. Two main results are presented: 1) FRI sources are less efficient than FRII in converting gravitational energy into radiation; 2) The accretion flow is an important X-ray component in all the FRII radio sources except for Low Excitation Line Radio galaxies (LEGs); LEGs have either the largest ratio between the jet kinetic (Lkin) and accretion power (Lacc) or strong absorption in X-rays.

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