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Three-dimensional hydrodynamical CO<sup>5</sup>BOLD model atmospheres of red giant stars III. Line formation in the atmospheres of giants located close to the base of the red giant branch.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 559, p. 1, doi. 10.1051/0004-6361/201321036
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- Article
Three-dimensional hydrodynamical CO<sup>5</sup>BOLD model atmospheres of red giant stars II. Spectral line formation in the atmosphere of a giant located near the RGB tip.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 549, p. 1, doi. 10.1051/0004-6361/201220240
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- Article
Can we trust elemental abundances derived in late-type giants with the classical 1D stellar atmosphere models?
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S265, p. 209, doi. 10.1017/S1743921310000566
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- Article
Entropy-calibrated stellar modeling: Testing and improving the use of prescriptions for the entropy of adiabatic convection.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202347700
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Abundance of strontium in the Galactic globular cluster 47 Tuc.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202347936
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- Article
Abundances of Mg and K in the atmospheres of turn-off stars in Galactic globular cluster 47 Tucanae.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 615, p. 1, doi. 10.1051/0004-6361/201731659
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- Article
Using the CIFIST grid of CO<sup>5</sup>BOLD 3D model atmospheres to study the effects of stellar granulation on photometric colours:II. The role of convection across the H-R diagram.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201732447
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- Article