Fig. 1.
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V-band Wide Field Imager (WFI) mosaic of the 30 Doradus region. O-type stars runaways single (red) and binary (green) identified in this work are spread throughout the field of view, while the non-runaway O-type stars (blue circles) cluster within the NGC 2060 and NGC 2070 OB associations (dashed 2.4′-radius circles, equiv. 36 pc in radius).
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