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All known Galactic Of?p stars have been shown to host strong, organized,magnetic fields. Recently, five Of?p stars have been discovered in theMagellanic Clouds. They posses photometric \citep{Naze} and spectroscopic\citep{Walborn} variability compatible with the Oblique Rotator Model (ORM).However, their magnetic fields have yet to be directly detected. We havedeveloped an algorithm allowing for the synthesis of photometric observablesbased on the Analytic Dynamical Magnetosphere (ADM) model of \citet{Owocki}. Weapply our model to OGLE photometry in order to constrain their magneticgeometries and surface dipole strengths. We predict that the field strengthsfor some of these candidate extra-Galactic magnetic stars may be within thedetection limits of the FORS2 instrument.

The Of?p stars of the Magellanic Clouds: Are they strongly magnetic?