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

Massive stars in young massive clusters insert tremendous amounts of mass andenergy into their surroundings in the form of stellar winds and supernovaejecta. Mutual shock-shock collisions lead to formation of hot gas, filling thevolume of the cluster. The pressure of this gas then drives a powerful clusterwind. However, it has been shown that if the cluster is massive and denseenough, it can evolve in the so--called bimodal regime, in which the hot gasinside the cluster becomes thermally unstable and forms dense clumps which aretrapped inside the cluster by its gravity. We will review works on the bimodalregime and discuss the implications for the formation of subsequent stellargenerations. The mass accumulates inside the cluster and as soon as a highenough column density is reached, the interior of the clumps becomesself-shielded against the ionising radiation of stars and the clumps collapseand form new stars. The second stellar generation will be enriched by productsof stellar evolution from the first generation, and will be concentrated nearthe cluster center.

Bimodal regime in young massive clusters leading to subsequent stellar generations