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What Governs Lorentz Factors of Jet Components in Blazars?

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Abstract

We use a sample of radio-loud Active Galactic Nuclei (AGNs) with measured black hole masses to explore the jet formation mechanisms in these sources. We find a significant correlation between black hole mass and the bulk Lorentz factor of the jet components for this sample, while no significant correlation is present between the bulk Lorentz factor and the Eddington ratio. Recent investigations suggested that the most super-massive black holes in elliptical galaxies have on average higher spins than the black holes in spiral galaxies. The correlation between black hole mass and bulk Lorentz factor of the jet components found in this work implies that the motion velocity of the jet components is probably governed by the black hole spin. The faster moving jets are magnetically accelerated by the magnetic fields threading the horizon of more rapidly rotating black holes.

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Acknowledgements

This work is supported by the National Basic Research Programme of China (grant 2009CB824800), the National Natural Science Foundation of China (grants 11173043, 11121062 and 11233006), and the Chinese Academy of Sciences (CAS)/State Administration of Foreign Experts Affairs (SAFEA) International Partnership Programme for Creative Research Teams (KJCX2-YW-T23).

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Correspondence to Xinwu Cao.

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Cao, X., Chai, B., Zhou, M. et al. What Governs Lorentz Factors of Jet Components in Blazars?. J Astrophys Astron 35, 357–362 (2014). https://doi.org/10.1007/s12036-014-9230-z

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  • DOI: https://doi.org/10.1007/s12036-014-9230-z

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