# The updated BaSTI stellar evolution models and isochrones: II. alpha-enhanced calculations

Pietrinferni, A, Hidalgo, SL, Cassisi, S, Salaris, M, Savino, A, Mucciarelli, A, Verma, D, Aguirre, VS, Aparicio, A and Ferguson, J The updated BaSTI stellar evolution models and isochrones: II. alpha-enhanced calculations. The Astrophysical Journal. ISSN 1538-4357 (Accepted)

 Text 2012.10085v1.pdf - Accepted Version Restricted to Repository staff only Download (1MB)

## Abstract

This is the second paper of a series devoted to present an updated release of the BaSTI ( a Bag of Stellar Tracks and Isochrones) stellar model and isochrone library. Following the publication of the updated solar scaled library, here we present the library for a $\alpha-$enhanced heavy element distribution. These new alpha-enhanced models account for all improvements and updates in the reference solar metal distribution and physics inputs, as in the new solar scaled library. The models cover a mass range between 0.1 and $15~M_{\odot}$, 18 metallicities between [Fe/H]=-3.20 and +0.06 with [alpha/Fe]=+0.4 , and a helium to metal enrichment ratio Delta{Y}\Delta{Z}=1.31. For each metallicity, He-enhanced stellar models are also provided. The isochrones cover (typically) an age range between 20Myr and 14.5Gyr, including consistently the pre-main sequence phase. Asteroseismic properties of the theoretical models have also been calculated. Models and isochrones have been compared with results from independent calculations, with the previous BaSTI release, and also with selected observations, to test the accuracy/reliability of these new calculations. All stellar evolution tracks, asteroseismic properties and isochrones are made publicly available at http://basti-iac.oa-teramo.inaf.it

Item Type: Article astro-ph.SR; astro-ph.SR Q Science > QB AstronomyQ Science > QC Physics Astrophysics Research Institute American Astronomical Society Author 04 Jan 2021 13:30 04 Jan 2021 13:30 https://researchonline.ljmu.ac.uk/id/eprint/14207

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