A Helical Magnetic Field in the jet of 3C 273(Session 1:Astrophysical Jets,High-Energy Emission from Accreting Compact Objects,Korea-Japan Seminar)
By K. Asada, M. Inoue, Y. Uchida, S. Kameno, K. Fujisawa, S. Iguchi, M. Mutoh. 2002
137 citations recorded by the source corpus.
Both in the Faraday Rotation Measure and the intrinsic polarization angle, new features are revealed to indicate a helical magnetic field operating along the jet of the bright active galactic nucleus 3C 273. The helical field has been suggested to be related to the formation and collimation of jets by magnetohydrodynamic models. The distribution of the rotation measure shows a systematic gradient with respect to the jet axis, which is expected by a helical magnetic field. In addition, the helical field can consistently explain two types in the direction of the projected magnetic field: parallel and perpendicular to the jet axis. Further, if the helical magnetic field is generated by winding up of an initial field by rotation of the accretion disk, we can uniquely determine the direction of the disk rotation, since the jet is approaching us.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/e9598997ff3ae4152ade7e2994c13afdd0501448
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Citations in the corpus
- Are Quasar Jets Dominated by Poynting Flux? (2005, background): “Such gradients have been found in several BL Lac objects (Gabuzda, Murray, & Cronin 2004) and in quasar 3C273 (Asada et al. 2002).”
- Helical magnetic fields associated with the relativistic jets of four BL Lac objects (2004, background): “Asada et al. (2002) claim to have detected such a gradient across the VLBI jet C© 2004 RAS, MNRAS 351, L89–L93 Helical fields in the jets of BL Lac objects L91 Table 1.”