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

Clusters are excellent test benches for verification and improvement ofstellar evolution theory. The recent detection of solar-like oscillations inG-K giants in the open cluster NGC6819 with Kepler provides us with independentconstraints on the masses and radii of stars on the red giant branch, as wellas on the distance to clusters and their ages. We present, for NGC6819,evolutionary models by considering rotation-induced mixing ; and thetheoretical low-l frequencies of our stellar models.

Constraining angular momentum transport processes in stellar interiors with red-giant stars in the open cluster NGC6819