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 Pro

Presents the zaia usage as premium feature

ZAIA

Presents AI Discovery search usage as a premium feature

AI Discovery

Presents AI Discovery explain and summary usage as a premium feature

Content Analysis

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Presents the pdf analysis as premium feature

PDF Analysis

1500 Top-up

3000 Top-up

Zendy Basic

2500 Top-up

Zendy Unlimited

Presents the access of premium content as premium feature

Premium Content

The Galactic halo has a complex assembly history, which can be seen in itswealth of kinematic and chemical substructure. Globular clusters lose starsthrough tidal interactions with the Galaxy and cluster evaporation processes,meaning that they are inevitably a source of halo stars. These "migrants" fromglobular clusters can be recognized in the halo field by the characteristiclight element abundance anticorrelations that are commonly observed only inglobular cluster stars, and the number of halo stars that can be chemicallytagged to globular clusters can be used to place limits on the formationpathways of those clusters.

Rediscovering the origins of the stellar halo with chemical tagging