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No Small Scale Radio Jets Here: Multi-Epoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA

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arxiv 2306.15047 v1 pith:BLPZY7NB submitted 2023-06-26 astro-ph.GA

classification astro-ph.GA
keywords radioobservationsvlbaemissionhostknotsobservedsystem
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We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations of the nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBA observations made on 1997 April 26. By cross-correlating the positions of emitting regions across both epochs, we find that spatially-resolved extra-nuclear radio knots in this system have sub-relativistic transverse speeds (v < 0.1c). We discuss sources of the observed knots and how the radio emission relates to additional phases of gas in the central ~150 pcs of this system. We suggest that the most likely explanation for the observed emission is synchrotron radiation formed by shocked host media via interactions between AGN winds and the host environment.

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Cited by 1 Pith paper

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

  1. Non-thermal emission in jets and winds: Expected emission and spectral index distributions

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

    Self-consistent CRE evolution in RMHD simulations produces distinct spectral-index gradients that distinguish compact AGN jets from winds even when morphology is ambiguous.

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