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

Young star clusters (SCs) are the cradle of stars and the site of importantdynamical processes. We present N-body simulations of young SCs includingrecipes for metal-dependent stellar evolution and mass loss by stellar winds.We show that metallicity affects significantly the collapse and post-corecollapse phase, provided that the core collapse timescale is of the same orderof magnitude as the lifetime of massive stars. In particular, the reversal ofcore collapse is faster for metal-rich SCs, where stellar winds are stronger.As a consequence, the half-mass radius of metal-poor SCs expands more than thatof metal-rich SCs.

Young star cluster evolution and metallicity