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Article

Yusof, N, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Eggenberger, P, Ekstrom, S, Georgy, C, Sibony, Y, Crowther, PA, Meynet, G, Kassim, HA, Harun, WAW, Maeder, A, Groh, JH, Farrell, E and Murphy, L (2022) Grids of stellar models with rotation VII: models from 0.8 to 300 M-circle dot at supersolar metallicity (Z=0.020). Monthly Notices of the Royal Astronomical Society, 511 (2). 2814 - 2828.

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.

Farrell, EJ, Groh, JH, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Murphy, L, Kaiser, E, Ekström, S, Georgy, C and Meynet, G (2020) Is GW190521 the merger of black holes from the first stellar generations? Monthly Notices of the Royal Astronomical Society, 502 (1). L40-L44.

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.

Groh, JH, Meynet, G, Georgy, C and Ekstrom, S (2013) Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death. Astronomy & Astrophysics, 558.

Georgy, C, Ekström, S, Eggenberger, P, Meynet, G, Haemmerlé, L, Maeder, A, Granada, A, Groh, JH, Hirschi, R, Mowlavi, N, Yusof, N, Charbonnel, C, Decressin, T and Barblan, F (2013) Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002. Astronomy & Astrophysics, 558.

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