(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.