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

Using the radiative transfer code Torus, we produce spectral-line cubes ofthe predicted HI profile from global SPH simulations of spiral galaxies. Torusgrids the SPH galaxy using Adaptive Mesh Refinement, then applies a ray-tracingmethod to infer the HI profile along the line(s) of sight. The gridded galaxycan be observed from any direction, which enables us to model the observed HIprofile for galaxies of any orientation. We can also place the observer insidethe galaxy, to simulate HI observations taken from the Earth's position in theMilky Way.

Synthetic Observations of the HI Line in SPH-Simulated Spiral Galaxies