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Article

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.

Groh, JH, Ekstroem, S, Georgy, C, Meynet, G, Choplin, A, Eggenberger, P, Hirschi, R, Maeder, A, Murphy, LJ, Boian, I and Fanell, EJ (2019) Grids of stellar models with rotation IV. Models from 1.7 to 120 M-circle dot at a metallicity Z=0.0004. Astronomy & Astrophysics, 627.

Frischknecht, U, Hirschi, R, Pignatari, M, Maeder, A, Meynet, G, Chiappini, C, Thielemann, F-K, Rauscher, T, Georgy, C and Ekstroem, S (2016) s-process production in rotating massive stars at solar and low metallicities. Monthly Notices of the Royal Astronomical Society, 456 (2). 1803 - 1825.

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