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/

Zendy Plus

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

Zendy Tools

Zendy Open

This paper reports one recent result from a set of pre-virialized galaxygroup simulations that are being used in an investigation of measurementtechniques for the quantity of intragroup light (IGL). We present evidence thatthe binding energy of the stellar material stripped from the galaxies isessentially uncorrelated with the local mass density. This suggests that IGLdetection methods based on the distribution of luminosity perform poorly indetecting the unbound stars.

Modeling the production of intergalactic light in the pre-collapse phase of galaxy groups