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Spectropolarimetric observations of HD 155806 - the hottest Galactic Oe star- were obtained with CFHT/ESPaDOnS to test the hypothesis that disk signaturesin its spectrum are due to magnetic channeling and confinement of its stellarwind. We did not detect a dipole field of sufficient strength to confine thewind, and could not confirm previous reports of a magnetic detection. Itappears that stellar magnetism is not responsible for producing the disk of HD155806.

Is the Wind of the Galactic Oe Star HD 155806 Magnetically Confined?