Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Ramalatswa, K. J."'
Autor:
Keszthelyi, Z., de Koter, A., Götberg, Y., Meynet, G., Brands, S. A., Petit, V., Carrington, M., David-Uraz, A., Geen, S. T., Georgy, C., Hirschi, R., Puls, J., Ramalatswa, K. J., Shultz, M. E., ud-Doula, A.
Magnetism can greatly impact the evolution of stars. In some stars with OBA spectral types there is direct evidence via the Zeeman effect for stable, large-scale magnetospheres, which lead to the spin-down of the stellar surface and reduced mass loss
Externí odkaz:
http://arxiv.org/abs/2211.07060
Autor:
Keszthelyi, Z., de Koter, A., Götberg, Y., Meynet, G., Brands, S. A., Petit, V., Carrington, M., David-Uraz, A., Geen, S. T., Georgy, C., Hirschi, R., Puls, J., Ramalatswa, K. J., Shultz, M. E., ud-Doula, A.
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:
http://arxiv.org/abs/2209.06350
Autor:
Keszthelyi, Z, de Koter, A, Götberg, Y, Meynet, G, Brands, S A, Petit, V, Carrington, M, David-Uraz, A, Geen, S T, Georgy, C, Hirschi, R, Puls, J, Ramalatswa, K J, Shultz, M E, ud-Doula, A
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Dec2022, Vol. 517 Issue 2, p2028-2055, 28p