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

Galaxy groups constitute the most common class of galaxy systems in the knownUniverse, unique in terms of environmental properties. However, despite recentadvances in optical and infrared observations as well as in theoreticalresearch, little is known about magnetic fields and the associated continuumradio emission. Studies on this issue have only been conducted in recent years,and many questions have yet to be resolved. This article aims to put the studyof group magnetism in a broader context, to present recent advances in thefield (mainly achieved with low-frequency radio interferometers), and to listthe issues that need to be addressed in future observations. To make it easierfor the Readers to get acquainted with the concepts presented in themanuscript, radio observations of two sample groups of galaxies are alsopresented.

galaxies

Somewhere in between: Tracing the Radio Emission from Galaxy Groups (or  Why Does the Future of Observing Galaxy Groups with Radio Telescopes Look  Promising?)