Observational View of Magnetic Fields in Active Galactic Nuclei Jets
2016 ◽
Vol 12
(S324)
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pp. 149-156
Keyword(s):
The Past
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AbstractAccording to the currently favored picture, relativistic jets in active galactic nuclei (AGN) are launched in the vicinity of the black hole by magnetic fields extracting energy from the spinning black hole or the accretion disk. In the past decades, various models from shocks to magnetic reconnection have been proposed as the energy dissipation mechanism in the jets. This paper presents a short review on how linear polarization observations can be used to constrain the magnetic field structure in the jets of AGN, and how the observations can be used to constrain the various emission models.
1990 ◽
Vol 140
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pp. 447-448
2017 ◽
Vol 467
(4)
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pp. 4526-4539
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2021 ◽
Vol 503
(1)
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pp. 1327-1344
2011 ◽
Vol 415
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pp. 2081-2092
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Keyword(s):
2009 ◽
Vol 702
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pp. L148-L152
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2014 ◽
Vol 23
(01)
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pp. 1450010
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Keyword(s):
Keyword(s):
2001 ◽
Vol 18
(3)
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pp. 215-220