English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

We present a case study of HE 0040-1105, an unobscured radio-quiet AGN at ahigh accretion rate (Eddington ratio = 0.19+/-0.04). This particular AGN hostsan ionized gas outflow with the largest spatial offset from its nucleuscompared to all other AGNs in the Close AGN Reference Survey (CARS). Bycombining multi-wavelength observations from VLT/MUSE, HST/WFC3, VLA, and EVNwe probe the ionization conditions, gas kinematics, and radio emission fromhost galaxy scales to the central few pc. We detect four kinematically distinctcomponents, one of which is a spatially unresolved AGN-driven outflow locatedwithin the central 500 pc, where it locally dominates the ISM conditions. Itsvelocity is too low to escape the host galaxy's gravitational potential, andmaybe re-accreted onto the central black hole via chaotic cold accretion. Wedetect compact radio emission in HE 0040-1105,within the region covered by theoutflow, varying on ~20 yr timescale. We show that neither AGN coronal emissionnor star formation processes wholly explain the radio morphology/spectrum. Thespatial alignment between the outflowing ionized gas and the radio continuumemission on 100 pc, scales is consistent with a weak jet morphology rather thandiffuse radio emission produced by AGN winds. > 90% of the outflowing ionizedgas emission originates from the central 100 pc, within which the ionizingluminosity of the outflow is comparable to the mechanical power of the radiojet. Although radio jets might primarily drive the outflow in HE 0040-1105,,radiation pressure from the AGN may contribute in this process.

The Close AGN Reference Survey (CARS): An interplay between radio jets and AGN radiation in the radio-quiet AGN HE 0040-1105