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Reading M87's DNA: A Double Helix revealing a large scale Helical Magnetic Field

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arxiv 2112.06971 v1 pith:NDMU7EP6 submitted 2021-12-13 astro-ph.GA astro-ph.HE

Reading M87's DNA: A Double Helix revealing a large scale Helical Magnetic Field

classification astro-ph.GA astro-ph.HE
keywords largeconfigurationfieldhelicalmagneticpolarizationscalesallow
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present unprecedented high fidelity radio images of the M87 jet. We analyzed Jansky Very Large Array (VLA) broadband, full polarization, radio data from 4 to 18 GHz. The observations were taken with the most extended configuration (A configuration), which allow the study of the emission of the jet up to kpc scales with a linear resolution $\sim$10 pc. The high sensitivity and resolution of our data allow to resolve the jet width. We confirm a double-helix morphology of the jet material between $\sim$300 pc and $\sim$1 kpc. We found a gradient of the polarization degree with a minimum at the projected axis and maxima at the jet edges, and a gradient in the Faraday depth with opposite signs at the jet edges. We also found that the behavior of the polarization properties along the wide range of frequencies is consistent with internal Faraday depolarization. All these characteristics strongly support the presence of a helical magnetic field in the M87 jet up to 1 kpc from the central black hole although the jet is most likely particle dominated at these large scales. Therefore, we propose a plausible scenario in which the helical configuration of the magnetic field has been maintained to large scales thanks to the presence of Kelvin-Helmholtz instabilities.

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Cited by 1 Pith paper

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  1. Helical radio jets as probes of magnetised cluster environments: Periodic Faraday Rotation Revealed in the Corkscrew Galaxy by POSSUM

    astro-ph.GA 2026-07 conditional novelty 6.5

    Periodic RM oscillations matching the Corkscrew jet's lateral deviations reveal a transition from jet/sheath to local-ICM Faraday media along the flow.