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Towards stellar effective temperatures and diameters at 1 per cent accuracy for future surveys
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ISOCHRONES FOR OLD (>5 GYR) STARS AND STELLAR POPULATIONS. I. MODELS FOR –2.4 ⩽ [Fe/H] ⩽+0.6, 0.25 ⩽Y⩽ 0.33, AND –0.4 ⩽ [α/Fe] ⩽+0.4
Improvements to stellar structure models, based on a grid of 3D convection simulations – I. T(τ) relations
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Properties of small-scale magnetism of stellar atmospheres
Oskar Steiner, René Salhab, Bernd Freytag, Paul Rajaguru, Werner Schaffenberger and Matthias Steffen Publications of the Astronomical Society of Japan 66(SP1) (2014) https://doi.org/10.1093/pasj/psu083
Planet transit and stellar granulation detection with interferometry
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars
Maria Bergemann GeoPlanet: Earth and Planetary Sciences, Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars 187 (2014) https://doi.org/10.1007/978-3-319-06956-2_17
A single low-energy, iron-poor supernova as the source of metals in the star SMSS J031300.36−670839.3
RADIAL STELLAR PULSATION AND THREE-DIMENSIONAL CONVECTION. III. COMPARISON OF TWO-DIMENSIONAL AND THREE-DIMENSIONAL CONVECTION EFFECTS ON RADIAL PULSATION