Fig. 4
Dependence of the interstellar polarization on distance in eastern, central, and western parts of the magnetic loop. Median lines are drawn for bins of 50 pc (in the distance range of 100−500 pc) and for 100 pc (up to 100 pc and beyond 500 pc). The plots show the polarizations of the stars whose error in the parallax estimation is ≤40%
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