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pro vyhledávání: '"Berry, I. D."'
Early-type B stars with strong magnetic fields and rapid rotation form centrifugal magnetospheres (CMs), as the relatively weak stellar wind becomes magnetically confined and centrifugally supported above the Kepler co-rotation radius. CM plasma is c
Externí odkaz:
http://arxiv.org/abs/2306.03990
Strongly magnetic, rapidly rotating B-type stars with relatively weak winds form centrifugal magnetospheres (CMs), as the stellar wind becomes magnetically confined above the Kepler co-rotation radius. Approximating the magnetic field as a dipole til
Externí odkaz:
http://arxiv.org/abs/2202.00615
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Apr2022, Vol. 511 Issue 4, p4815-4825, 11p