Zlatibor, Serbia, 23-27 April 2017
A relation of jet power to the central black hole and its accretion
1 Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi 830011, PR China
2 Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, PR China
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Published online: 9 December 2013
We have developed an integrated jet power formula in the context of the Blandford-Znajek and Blandford-Payne models, and applied this model to the Foschini sample. The result suggests that there is a positive correlation of the jet power versus the product of the disk luminosity and black hole mass within each type of source, and the di↵erent linear correlation slopes imply that the disk emissivity efficiency and/or the SMBH spin are quite di↵erent for FSRQs, BL Lacs and γ – NLS 1s.
© Owned by the authors, published by EDP Sciences, 2013
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