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Predictions for Gravity-mode Periods and Surface Abundances in Intermediate-mass Dwarfs from Shear Mixing and Radiative Levitation
Joey S. G. Mombarg, Aaron Dotter, Michel Rieutord, Mathias Michielsen, Timothy Van Reeth and Conny Aerts The Astrophysical Journal 925(2) 154 (2022) https://doi.org/10.3847/1538-4357/ac3dfb
Stellar models with self-consistent Rosseland opacities
On the first δ Sct–roAp hybrid pulsator and the stability of p and g modes in chemically peculiar A/F stars
Simon J Murphy, Hideyuki Saio, Masahide Takada-Hidai, et al. Monthly Notices of the Royal Astronomical Society 498(3) 4272 (2020) https://doi.org/10.1093/mnras/staa2667
Asteroseismic Modeling of Gravity Modes in Slowly Rotating A/F Stars with Radiative Levitation
Joey S. G. Mombarg, Aaron Dotter, Timothy Van Reeth, Andrew Tkachenko, Sarah Gebruers and Conny Aerts The Astrophysical Journal 895(1) 51 (2020) https://doi.org/10.3847/1538-4357/ab8d36
The Axial Rotation and Variable Macroturbulence of RR Lyrae and Red Horizontal Branch Stars
George W. Preston, Christopher Sneden, Merieme Chadid, Ian B. Thompson and Stephen A. Shectman The Astronomical Journal 157(4) 153 (2019) https://doi.org/10.3847/1538-3881/ab0ae1
Progress in Global Helioseismology: A New Light on the Solar Modeling Problem and Its Implications for Solar-Like Stars
Impacts of radiative accelerations on solar-like oscillating main-sequence stars
M. Deal, G. Alecian, Y. Lebreton, M. J. Goupil, J. P. Marques, F. LeBlanc, P. Morel and B. Pichon Astronomy & Astrophysics 618 A10 (2018) https://doi.org/10.1051/0004-6361/201833361
Role of atomic diffusion in the opacity enhancement inside B-type stars
Pulsation versus metallicism in Am stars as revealed by LAMOST and WASP
B. Smalley, V. Antoci, D. L. Holdsworth, D. W. Kurtz, S. J. Murphy, P. De Cat, D. R. Anderson, G. Catanzaro, A. Collier Cameron, C. Hellier, P. F. L. Maxted, A. J. Norton, D. Pollacco, V. Ripepi, R. G. West and P. J. Wheatley Monthly Notices of the Royal Astronomical Society 465(3) 1 (2017) https://doi.org/10.1093/mnras/stw2903
Important consequences of atomic diffusion inside main-sequence stars: opacities, extra-mixing, oscillations