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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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Photometric survey identifies 137 PMS stars with median accretion rate 8e-9 solar masses per year whose accretion properties correlate with distance from nearby hot stars, suggesting UV disc erosion.
citing papers explorer
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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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Photometric determination of the mass accretion rates of pre-main sequence stars. IX. Recent star formation in the periphery of NGC 346
Photometric survey identifies 137 PMS stars with median accretion rate 8e-9 solar masses per year whose accretion properties correlate with distance from nearby hot stars, suggesting UV disc erosion.