Fig. C.3.
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Extinction of the H II knots in the stripped material of NGC 3314A derived from the best NEBULABAYES fit as function of their distance from UDG 32, with the same colour-coding as Fig. 2. The red dashed horizontal line denotes the typical extinction values in the interspersed dusty arms of NGC 3314A (Keel & White 2001). For convenience, the top axis shows the approximate distance to NGC 3314A.
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