scholarly journals Transverse Faraday-rotation gradients across the jets of 15 active galactic nuclei

2015 ◽  
Vol 450 (3) ◽  
pp. 2441-2450 ◽  
Author(s):  
D. C. Gabuzda ◽  
S. Knuettel ◽  
B. Reardon
2017 ◽  
Vol 472 (2) ◽  
pp. 1792-1801 ◽  
Author(s):  
D. C. Gabuzda ◽  
N. Roche ◽  
A. Kirwan ◽  
S. Knuettel ◽  
M. Nagle ◽  
...  

2012 ◽  
Vol 144 (4) ◽  
pp. 105 ◽  
Author(s):  
Talvikki Hovatta ◽  
Matthew L. Lister ◽  
Margo F. Aller ◽  
Hugh D. Aller ◽  
Daniel C. Homan ◽  
...  

2013 ◽  
Vol 431 (1) ◽  
pp. 695-709 ◽  
Author(s):  
M. Mahmud ◽  
C. P. Coughlan ◽  
E. Murphy ◽  
D. C. Gabuzda ◽  
D. R. Hallahan

2008 ◽  
Vol 17 (09) ◽  
pp. 1521-1530 ◽  
Author(s):  
D. C. GABUZDA

A growing number of jets in active galactic nuclei (AGN) show clear signs of helical magnetic (B) fields: Faraday-rotation gradients across the VLBI jets, extended regions of jet with orthogonal B fields, transverse polarization and total-intensity structures characteristic of helical fields, interknot polarization implying underlying orthogonal B fields, and a predominance of orthogonal B fields in the VLBI cores. In addition, a link has now been found between the circular polarization detected in AGN cores and the presence of helical jet B fields within these cores. This now abundant evidence compels us to take very seriously the idea that many, possibly all, AGN jets have helical B fields. As a whole, the recent observational results considered here suggest that we must look at AGN jets as fundamentally electromagnetic, current-carrying structures if we wish to fully understand their nature. This provides an overall framework for interpreting various observed phenomena associated with the relativistic jets of AGN, including high-energy phenomena. Superposed on the structure of the underlying helical B field may be the effects of relativistic shocks and interaction with the surrounding medium in some cases; these may dominate observed phenomena locally, while it is the "intrinsic" helical B field of the jet itself that determines the global observed characteristics of the jet.


Galaxies ◽  
2021 ◽  
Vol 9 (3) ◽  
pp. 51
Author(s):  
Iván Martí-Vidal ◽  
Ciriaco Goddi

The linear polarization of non-thermal emission encodes information about the structure of the magnetic fields, either from the region where the emission is produced (i.e., the intrinsic polarization angle) and/or from the screens of magnetized plasma that may be located on its way towards Earth (i.e., the effect of Faraday rotation). In addition, the variability timescale of the polarized emission, or its Faraday rotation, can be used to estimate the size of the region where the emission (or the Faraday rotation) originates. The observation of polarized emission from active galactic nuclei (AGN) and, in particular, its time evolution, also provides information about the critical role that magnetic fields may play in the process of jet launching and propagation. In this paper, we review some recent results about polarization variability from the cores of AGN jets, including observations at high spatial resolutions and/or at high radio frequencies.


2013 ◽  
Vol 145 (6) ◽  
pp. 172 ◽  
Author(s):  
Talvikki Hovatta ◽  
Matthew L. Lister ◽  
Margo F. Aller ◽  
Hugh D. Aller ◽  
Daniel C. Homan ◽  
...  

2010 ◽  
Vol 6 (S274) ◽  
pp. 258-262
Author(s):  
Oliver Porth

AbstractWe perform axisymmetric simulations of two-component jet acceleration using the special relativistic MHD code PLUTO (Mignone et al., 2007). The inner, thermally driven component constitutes a dilute relativistic plasma originating in a high enthalpy central corona. The second component is a Poynting-dominated wind driven by a global current system. Once a near-stationary state is reached, we solve the polarized Synchrotron radiation transport incorporating self-absorption and (internal) Faraday rotation. With this approach we obtain high-resolution radio maps and spectra that can help in the interpretation of observational data from nearby active galactic nuclei by predicting spine-sheath polarization structures and Faraday rotation gradients.


Galaxies ◽  
2018 ◽  
Vol 6 (2) ◽  
pp. 40
Author(s):  
Alice Pasetto ◽  
Carlos Carrasco-González ◽  
Shane O’Sullivan ◽  
Aritra Basu ◽  
Gabriele Bruni ◽  
...  

2004 ◽  
Vol 600 (1) ◽  
pp. 88-95 ◽  
Author(s):  
Yutaka Uchida ◽  
Hiromitsu Kigure ◽  
Shigenobu Hirose ◽  
Masanori Nakamura ◽  
Robert Cameron

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