Fig. 3.
MUSE vs. HST images of 4 × 4 arcsec2 size from field (i), as examples of the star in the center being affected by different severity of crowding. a/b: ID1154, A1 Ib star, unblended. c/d: ID1179, B3 III star, negligible blending. e/f: ID995, central star cluster in bright H II region, spectrum heavily affected by blending and nebular emission, no reliable classification possible.
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