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Fig. 6.

K-band spectra of candidate runaways (black) compared to members of the Arches and Quintuplet (red; Clark et al. 2018a,b). [DCW2011] P96 and P97 show a close resemblance to WN7-8h and O6-7 Ia+ stars within the Arches, while [DCW2011] P19 corresponds to the sole broad-lined WN9h star within the older Quintuplet.
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