Using ZDI maps to determine magnetic forces and torques at the photospheres of Early-type stars
Using ZDI maps to determine magnetic forces and torques at the photospheres of Early-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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We use the magnetic field components measured by Zeeman Doppler imaging (ZDI) to calculate the stellar surface force and torque due to magnetic stresses for the fast rotators \(\sigma\) Ori E, 36 Lyn and CU Vir, and the slow rotator \(\tau\) Sco. If we assume the stars have spherical photospheres, the estimated torques give spin down time scales no...
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Using ZDI maps to determine magnetic forces and torques at the photospheres of Early-type stars
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TN_cdi_proquest_journals_3040140515
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3040140515
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2331-8422
