Fig. 14
Polarized flux profile ⟨ P | x | ⟩ of the AU Mic debris disk derived from the polarimetric profiles of Graham et al. (2007, their Fig. 4). The bins are 5 AU wide and error bars are obtained from error propagation including systematic uncertainties. Open circles are derived from noisy data without considering the bias effect for the determination of the fractional polarization (Clarke et al. 1983).
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