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

The static pressure of the hot gas that fills clusters and groups of galaxiescan affect significantly the volume density and thickness of the gas disks ingalaxies. In combination with the dynamic pressure, the static pressure allowsseveral observed peculiarities of spiral galaxies surrounded by a hot medium tobe explained.

Static Pressure of Hot Gas: Its Effect on the Gas Disks of Galaxies