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Fig. 4
Interstellar polarization according to dust phase abundance of iron. Halo stars with |b| > 30° and disk stars with |b| ≤ 30° and low (E(B − V) ≤ 0.2) and high (E(B − V) > 0.2) reddening are shown with different symbols. The number of stars is indicated in parentheses in the legend.
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