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 Plus annual

Presents the access of premium content as premium feature

Premium Content

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 annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We produce radiation hydrodynamics models of an AGN 'torus' plus outflow on1-100 pc scales. This large scale permits direct comparison with observations,provides justification for configurations used in radiation transfer models,and tests the sensitivity of results of smaller scale dynamical models. We findthat anisotropic radiation from an AGN accretion disk can cause an outflow toevolve to become more polar, agreeing with the ubiquity of polar extendedmid-IR emission, and the general geometry predicted by radiative transfermodels. We also find the velocity maps can reproduce many features ofobservations, including apparent 'counter-rotation'.

Radiation hydrodynamics models of Active Galactic Nuclei: Beyond the central parsec