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

Core overshoot is a large source of uncertainty in constructing stellarmodels. Whether the amount of overshoot is constant or mass dependent is notcompletely known, even though models sometimes assume a mass-based trend. Inthis work we use asteroseismic data from stars observed by \textit{Kepler} toinvestigate the relationship between various stellar properties and the amountof overshoot needed to properly model a given star. We find a strong positivetrend between stellar mass and overshoot amount for stars between 1.1 and 1.5$M_\odot$, with a slope of 0.89. Additionally, we investigate how inferredstellar properties change as a function of overshoot. Our model grids show thatthe inferred stellar mass and radius can vary by as much as 14\% and 6\%respectively, depending on the extent of overshoot. This mass spread results ina commensurate spread in the ages.

Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology