Modelling the Magnetic Fields and Magnetospheres of Early B-Type Stars
Modelling the Magnetic Fields and Magnetospheres of Early B-Type Stars
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The powerful radiative winds of hot stars with strong magnetic fields are magnetically confined into large, corotating magnetospheres, which exert important influences on stellar evolution via rotational spindown and mass-loss quenching. They are detectable via diagnostics across the electromagnetic spectrum. Since the fossil magnetic fields of ear...
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Modelling the Magnetic Fields and Magnetospheres of Early B-Type Stars
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TN_cdi_proquest_journals_2328519755
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2328519755
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E-ISSN
2331-8422
