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pro vyhledávání: '"K J Ramalatswa"'
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
https://lirias.kuleuven.be/handle/20.500.12942/706503