EPJ Web of Conferences
Volume 61, 2013The Innermost Regions of Relativistic Jets and Their Magnetic Fields
|Number of page(s)||2|
|Published online||09 December 2013|
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
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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