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Fig. 4.
Blueward part of the MUSE spectrum of the extracted central source of the H II region in Leo P (LP 26). The identified emission lines, from left-to-right by species, are: Hβ; He I λ λ4713,4922,5016; [O III] λ λ4959,5007. The He II λ λ4686, 5411 absorption lines provide the first direct evidence for an O-type star in Leo P.
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