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arXiv · 2401.06698

Core shift in parabolic accelerating jets

Nokhrina E. E.·Pushkarev A. B
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Abstract

The core shift method is a powerful method to estimate the physical parameters in relativistic jets from active galactic nuclei. The classical approach assumes a conical geometry of a jet and a constant plasma speed. However, recent observations showed that neither may hold close to the central engine, where plasma in a jet is effectively accelerating, and the jet geometry is quasi-parabolic. We modify the classical core shift method to account for these jet properties. We show that the core shift index may assume values in the range 0.8-1.2 or 0.53-0.8 depending on the jet geometry and viewing angle, with the indices close to both values are indeed being observed. We obtain the expressions to estimate jet magnetic field and a total magnetic flux in a jet. We show that the obtained magnetic field value can be easily recalculated down to the gravitational radius scales. For M 87 and NGC 315 these values are in good agreement with the ones obtained by different methods.

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Nokhrina E. E., Pushkarev A. B. 2024-01-12. Core shift in parabolic accelerating jets. https://doi.org/10.1093/mnras%2Fstae179

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