Stellar feedback in M 83 as observed with MUSE - II. Analysis of the H II region population: Ionisation budget and pre-SN feedback

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Fig. A.1.

Emission peaks (black ‘+’) and boundaries (thin black lines) of regions identified in a large H II complex with three different values of the f_noise parameter (Eq. 1). The thick black contours indicate the SB threshold adopted for the H II regions (see Sect. 3.1).

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