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Radio Jet-Ambient Medium Interactions on Parsec Scales in the Blazar 1055+018

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arxiv astro-ph/9903330 v3 pith:DTWVX7IR submitted 1999-03-22 astro-ph

classification astro-ph
keywords magneticblazarsboundaryfieldlayermediumpolarizationspine
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As part of our study of the magnetic fields of AGN we have recently observed a large sample of blazars with the Very Long Baseline Array. Here we report the discovery of a striking two-component jet in the source 1055+018, consisting of an inner spine with a transverse magnetic field, and a fragmentary but distinct boundary layer with a longitudinal magnetic field. The polarization distribution in the spine strongly supports shocked-jet models while that in the boundary layer suggests interaction with the surrounding medium. This behavior suggests a new way to understand the differing polarization properties of strong- and weak-lined blazars.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dissipation and particle acceleration in astrophysical jets with velocity and magnetic shear: Interaction of Kelvin-Helmholtz and Drift-Kink Instabilities

    astro-ph.HE 2025-01 conditional novelty 7.0 of 10

    Combined velocity and magnetic shear in a relativistic pair plasma drives interacting Kelvin-Helmholtz and drift-kink instabilities that enhance dissipation and produce nonthermal particle acceleration.

  2. Polarization Architecture of Steady GRMHD Jets from the Horizon to Infinity

    astro-ph.HE 2026-07 unverdicted novelty 6.0 of 10

    Steady GRMHD jets exhibit a universal near-horizon polarization pattern set only by black hole spin, with large-radius polarization angle following a collimation-determined power law and intermediate scales modified b...

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