Raw (uncorrected for the underlying stellar PSF) Intensity and Polarized Intensity maps of IRC+10420 at 2.2 microns using MMTPol (Shenoy et al. 2015, submitted). The centeral star at these wavelengths severely satruates. The resolution of MMTPol for these observations was FWHM = 0.2". Note how clearly the face-on circumstellar disk shows up in polarized intensity.