Keele Research Repository

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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.

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.

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).

Scott, LJA, Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522, Georgy, C, Arnett, WD, Meakin, C, Kaiser, EA, Ekström, S and Yusof, N (2021) Convective core entrainment in 1D main-sequence stellar models. Monthly Notices of the Royal Astronomical Society, 503 (3). 4208 - 4220.

Gilmer, MS, Kozyreva, A, Hirschi, R, Fröhlich, C and Yusof, N (2017) Pair-instability Supernova Simulations: Progenitor Evolution, Explosion, and Light Curves. Astrophysical Journal, 846 (2). 100 - 100.

Whalen, DJ, Smidt, J, Heger, A, Hirschi, R, Yusof, N, Even, W, Fryer, CL, Stiavelli, M, Chen, K-J and Joggerst, CC (2014) Pair-instability supernovae in the local universe. Astrophysical Journal, 797 (1).

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.

Yusof, N, Hirschi, R, Meynet, G, Crowther, PA, Ekstrom, S, Frischknecht, U, Georgy, C, Kassim, HA and Schnurr, O (2013) Evolution and fate of very massive stars. Monthly Notices of the Royal Astronomical Society, 433 (2). pp. 1114-1132.

Crowther, PA, Hirschi, R, Walborn, NR and Yusof, N (2012) Very massive stars and the Eddington Limit.

Crowther, PA, Schnurr, O, Hirschi, R, Yusof, N, Parker, RJ, Goodwin, SP and Kassim, HA (2010) The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit. Monthly Notices of the Royal Astronomical Society, 408 (2). 731 -751.