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

Multiple stellar populations in the Milky Way globular clusters manifestthemselves with a large variety. Although chemical abundance variations inlight elements, including He, are ubiquitous, the amount of these variations isdifferent in different globulars. Stellar populations with distinct Fe, C+N+Oand slow-neutron capture elements have been now detected in some globularclusters, whose number will likely increase. All these chemical featurescorrespond to specific photometric patterns. I review the chemical+photometricfeatures of the multiple stellar populations in globular clusters and discusshow the interpretation of data is being more and more challenging. Veryexcitingly, the origin and evolution of globular clusters is being a complexpuzzle to compose.

Chemical abundances of multiple stellar populations in massive globular clusters