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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Recent ALMA observations have resolved the obscuring torus in the nearest Sy2galaxy, NGC1068, in the millimeter band. These observations have confirmed thepresence of a geometrically thick torus with an orbital motion of its matterand the velocity distribution which can reflect the clumpy structure. In theframework of N-body simulations we consider a dynamical model of an obscuringtorus which accounts for the gravitational interaction between the cloudsmoving in the field of the central mass. In considered model, clouds areorbiting around the central mass exhibiting a spread in inclination andeccentricity. The self-gravity of the torus induces the velocity distributionof clouds with a global orbital motion which mimics the ALMA data for NGC1068.

Interpretation of ALMA velocity map for the obscuring torus in NGC1068