Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asthe..97..687a&link_type=abstract
The Astronomical Herald (ISSN 0374-2466), Vol. 97, No. 12, p. 687 - 693 (2004)
Astronomy and Astrophysics
Astronomy
Active Galactic Nuclei, Jets, Magnetic Fields
Scientific paper
In order to reveal 3D structure of a magnetic field in AGN jets, we analyzed archival data observed with VLBA polarimetry towards 3C 273 jet. We found a curious gradient with respect to the jet axis in the distribution of Faraday Rotation Measure. The distribution is well-explained by helical magnetic field, which is related to the formation and collimation mechanism of jets by magnetohydrodynamic models. With assuming MHD model, we can uniquely determine the direction of the disk rotation.
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