Populations of rotating stars - I. Models from 1.7 to 15 M⊙ at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1
A&A, 553 (2013) A24
Published online: 2013-04-25
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A machine-learning photometric classifier for massive stars in nearby galaxies
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The Role of Binarity and Stellar Rotation in the Split Main Sequence of NGC 2422
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The wide upper main sequence and main-sequence turnoff of the ∼ 800 Myr old star cluster NGC 1831
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TESS survey of rotational and pulsational variability of mercury–manganese stars
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Constraining axion-like particles using the white dwarf initial-final mass relation
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Probing the interior physics of stars through asteroseismology
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Massive Star Modeling and Nucleosynthesis
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$$\varvec{U\!BV\!I}$$ CCD photometry of Berkeley 55 open cluster
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Convective core sizes in rotating massive stars
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Fundamental parameters and non‐local thermodynamic equilibrium abundances of key light elements for nine bright and nearby K giants
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Refined fundamental parameters of Canopus from combined near-IR interferometry and spectral energy distribution
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Outbursts and stellar properties of the classical Be star HD 6226
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