MIST provides a new publicly available grid of solar-scaled stellar isochrones and evolutionary tracks computed self-consistently with MESA from pre-main sequence through advanced stages for masses 0.1-300 solar masses and metallicities -2 to 0.5.
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Veiling-corrected lithium abundances in eight young clusters peak at 3.3-3.8 dex with upper age limits of ~5 Myr, alongside slightly sub-solar iron and barium overabundances up to 0.75 dex.
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MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
MIST provides a new publicly available grid of solar-scaled stellar isochrones and evolutionary tracks computed self-consistently with MESA from pre-main sequence through advanced stages for masses 0.1-300 solar masses and metallicities -2 to 0.5.
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PENELLOPE: IX. Lithium, iron and barium elemental abundances in eight nearby young clusters
Veiling-corrected lithium abundances in eight young clusters peak at 3.3-3.8 dex with upper age limits of ~5 Myr, alongside slightly sub-solar iron and barium overabundances up to 0.75 dex.