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Martinet, S, Meynet, G, Nandal, D, Ekstrom, S, Georgy, C, Haemmerle, L, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Yusof, N, Gounelle, M and Dwarkadas, V (2022) Very massive star winds as sources of the short-lived radioactive isotope Al-26. Astronomy and Astrophysics: a European journal, 664.
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.
Murphy, LJ, Groh, JH, Ekstrom, S, Meynet, G, Pezzotti, C, Georgy, C, Choplin, A, Eggenberger, P, Farrell, E, Haemmerle, L, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Maeder, A and Martinet, S (2021) Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity. Monthly Notices of the Royal Astronomical Society, 501 (2). pp. 2745-2763.