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Eggenberger, P, Ekstroem, S, Georgy, C, Martinet, S, Pezzotti, C, Nandal, D, Meynet, G, Buldgen, G, Salmon, S, Haemmerle, L, Maeder, A, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Yusof, N, Groh, J, Farrell, E, Murphy, L and Choplin, A (2021) Grids of stellar models with rotation VI. Models from 0.8 to 120 M-circle dot at a metallicity Z=0.006. Astronomy & Astrophysics, 652 (A137).
Martinet, S, Meynet, G, Ekstroem, S, Simon-Diaz, S, Holgado, G, Castro, N, Georgy, C, Eggenberger, P, Buldgen, G, Salmon, S, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Groh, J, Farrell, E and Murphy, L (2021) Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars. Astronomy and Astrophysics, 648.
Rendle, BM, Buldgen, G, Miglio, A, Reese, D, Noels, A, Davies, GR, Campante, TL, Chaplin, WJ, Lund, MN, Kuszlewicz, JS, Scott, LJA ORCID: https://orcid.org/0000-0001-8696-7981, Scuflaire, R, Ball, WH, Smetana, J and Nsamba, B (2019) AIMS – a new tool for stellar parameter determinations using asteroseismic constraints. Monthly Notices of the Royal Astronomical Society, 484 (1). pp. 771-786.