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

The dynamics of a galactic disk in a non-axisymmetric (triaxial) dark halo isstudied in detail using high-resolution, numerical, hydrodynamical models. Along-lived, two-armed spiral pattern is generated for a wide range ofparameters. The spiral structure is global, and the number of turns can be twoor three, depending on the model parameters. The morphology and kinematics ofthe spiral pattern are studied as functions of the halo and disk parameters.The spiral structure rotates slowly, and its angular velocity variesquasi-periodically. Models with differing relative halo masses, halo semi-axisratios, distributions of matter in the disk, Mach numbers in the gaseouscomponent, and angular rotational velocities of their halos are considered.

Dynamics of Gaseous Disks in a Non-axisymmetric Dark Halo