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

We explore the role of mass loss and convective core overshoot in theevolution of Classical Cepheids. Stellar evolution models are computed with arecipe for pulsation-driven mass loss and it is found that mass loss alone isunable to account for the long-standing Cepheid mass discrepancy. However, thecombination of mass loss and moderate convective core overshooting does providea solution, bringing the amount of convective core overshooting in Cepheidscloser to that found for other stars.

Convective Core Overshoot & Mass Loss in Classical Cepheids: A Solution to the Mass Discrepancy?