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Paper: X-ray Emission and Incidence of Magnetic Fields in Massive Stars of the Orion Nebula Cluster
Volume: 405, Solar Polarization 5: In Honor of Jan Olof Stenflo
Page: 547
Authors: Petit, V.; Wade, G.A.; Drissen, L.; Montmerle, T.
Abstract: Magnetic fields have been frequently invoked as a likely source of variability and confinement of the winds of the Orion Nebula Cluster massive stars. We carried out sensitive ESPaDOnS observations to search for direct evidence of such fields, detecting unambiguous Zeeman signatures in three objects
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