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

We present a large grid of stellar evolutionary tracks, which are suitable tomodelling star clusters and galaxies by means of population synthesis. Thetracks are presented for the initial chemical compositions [Z=0.0004, Y=0.23],[Z=0.001, Y=0.23], [Z=0.004, Y=0.24], [Z=0.008, Y=0.25], [Z=0.019, Y=0.273](solar composition), and [Z=0.03, Y=0.30]. They are computed with updatedopacities and equation of state, and a moderate amount of convective overshoot.The range of initial masses goes from 0.15 M_sun to 7 M_sun, and theevolutionary phases extend from the zero age main sequence (ZAMS) till eitherthe thermally pulsing AGB regime or carbon ignition. We also present anadditional set of models with solar composition, computed using the classicalSchwarzschild's criterion for convective boundaries. From all these tracks, wederive the theoretical isochrones in the Johnson-Cousins UBVRIJHK broad-bandphotometric system.

Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 $M_{\odot}$, and from $Z=0.0004$ to 0.03