Progress on nuclear reaction rates affecting the stellar production of 26Al

Autor: A M Laird, M Lugaro, A Kankainen, P Adsley, D W Bardayan, H E Brinkman, B Côté, C M Deibel, R Diehl, F Hammache, J W den Hartogh, J José, D Kurtulgil, C Lederer-Woods, G Lotay, G Meynet, S Palmerini, M Pignatari, R Reifarth, N de Séréville, A Sieverding, R J Stancliffe, T C L Trueman, T Lawson, J S Vink, C Massimi, A Mengoni

Publikováno v: Laird, A M, Lugaro, M, Kankainen, A, Adsley, P, Bardayan, D W, Brinkman, H E, Cote, B, Deibel, C M, Diehl, R, Hammache, F, den Hartogh, J W, Jose, J, Kurtulgil, D, Lederer-Woods, C, Lotay, G, Meynet, G, Palmerini, S, Pignatari, M, Reifarth, R, de Sereville, N, Sieverding, A, Stancliffe, R J, Trueman, T C L, Lawson, T, Vink, J S, Massimi, C & Mengoni, A 2023, ' Progress on nuclear reaction rates affecting the stellar production of 26Al ', Journal of Physics G: Nuclear and Particle Physics, vol. 50, no. 3, 033002, pp. 1-59 . https://doi.org/10.1088/1361-6471/ac9cf8
Journal of Physics G

The radioisotope 26Al is a key observable for nucleosynthesis in the Galaxy and the environment of the early Solar System. To properly interpret the large variety of astronomical and meteoritic data, it is crucial to understand both the nuclear react

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d502ee7a275a6460e5c553a762f1d72a
https://hdl.handle.net/2117/385964

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Evolution of rotating massive stars with new hydrodynamic wind models

Autor: A. C. Gormaz-Matamala, J. Cuadra, G. Meynet, M. Curé

Mass loss due to line-driven winds is central to our understanding of the evolution of massive stars. We extend the evolution models introduced in Paper I, where the mass loss recipe is based on the simultaneous calculation of the wind hydrodynamics

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b039f63e4450273231dcd49d49d7641d
http://arxiv.org/abs/2303.13058

The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities

Autor: Z Keszthelyi, A de Koter, Y Götberg, G Meynet, S A Brands, V Petit, M Carrington, A David-Uraz, S T Geen, C Georgy, R Hirschi, J Puls, K J Ramalatswa, M E Shultz, A ud-Doula

Publikováno v: Monthly Notices of the Royal Astronomical Society, 517(2), 2028-2055. Oxford University Press

Magnetic fields can drastically change predictions of evolutionary models of massive stars via mass-loss quenching, magnetic braking, and efficient angular momentum transport, which we aim to quantify in this work. We use the MESA software instrument

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41ed4858dd8b05fdbe9150cbe77feb7d
https://lirias.kuleuven.be/handle/20.500.12942/706503