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 present a numerical code for multi-component simulation of the galacticevolution. Our code includes the following parts: $N$-body is used to evolvedark matter, stellar dynamics and dust grains, gas dynamics is based onTVD-MUSCL scheme with the extra modules for thermal processes, star formation,magnetic fields, chemical kinetics and multi-species advection. We describe ourcode in brief, but we give more details for the magneto-gas dynamics. Wepresent several tests for our code and show that our code have passed the testswith a reasonable accuracy. Our code is parallelized using the MPI library. Weapply our code to study the large scale dynamics of galactic discs.

Numerical code for multi-component galaxies: from N-body to chemistry and magnetic fields