University of Hertfordshire

From the same journal

From the same journal

By the same authors

3D Hydrodynamic Simulations of Large-Scale Precessing Jets: Radio Morphology

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  • staa3020

    Accepted author manuscript, 1.92 MB, PDF document

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Original languageEnglish
Article numberstaa3020
JournalMonthly Notices of the Royal Astronomical Society
Early online date2 Oct 2020
DOIs
Publication statusE-pub ahead of print - 2 Oct 2020

Abstract

The prospect of relativistic jets exhibiting complex morphologies as a consequence of geodetic precession has long been hypothesised. We have carried out a 3D hydrodynamics simulation study varying the precession cone angle, jet injection speed and number of turns per simulation time. Using proxies for the radio emission we project the sources with different inclinations to the line of sight to the observer. We find that a number of different precession combinations result in characteristic `X' shaped sources which are frequently observed in radio data, and some precessing jet morphologies may mimic the morphological signatures of restarting radio sources. We look at jets ranging in scale from tens to hundreds of kiloparsecs and develop tools for identifying known precession indicators of point symmetry, curvature and jet misalignment from the lobe axis and show that, based on our simulation sample of precessing and non-precessing jets, a radio source that displays any of these indicators has a 98% chance of being a precessing source.

Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society] ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. The final published version is available at: https://doi.org/10.1093/mnras/staa3020.

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