AGN jet physics from measurements of the frequency-dependent position of the VLBI radio core
Shane P. O'Sullivan, Denise C. Gabuzda

TL;DR
This study measures the frequency-dependent position shifts of VLBI radio cores to derive physical parameters like magnetic field strength and core distance, using a cross-correlation alignment method validated against phase-referencing.
Contribution
It introduces a cross-correlation technique for aligning VLBI images to accurately measure core shifts, enabling precise estimation of magnetic fields and core locations in AGN jets.
Findings
Magnetic field strength of 0.15 G in Mrk 501 at 8.4 GHz.
Estimated magnetic fields of ~1 G in millimeter VLBI cores.
Core distances ranging from 0.8 to 20 pc depending on frequency and source.
Abstract
Accurate measurement of the frequency-dependent shift of the self-absorbed radio core is required for multi-frequency analysis of VLBI data since absolute positional information is lost as a result of phase self-calibration. We use the cross-correlation technique of Croke & Gabuzda (2008) on the optically thin jet emission to align our VLBA images. Our results are consistent with those obtained from the phase-referencing method, as well as alignment by model-fitted optically thin jet components. Physical parameters of the compact jet regions, such as the magnetic field strength (B_core) and the distance of the radio core to the jet origin (r_core), can be calculated from these measurements. For the source Mrk 501, we find a magnetic field strength of 0.15\pm0.04 G in the 8.4-GHz core at a distance of 0.8\pm0.2 pc from the base of the jet. By extrapolating our 4.6 to 15.4 GHz results for…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Precipitation Measurement and Analysis
