The core mass function in 30Dor-10 is consistent with a Salpeter-like slope, implying that stellar IMF variations in extreme environments result from evolutionary processes rather than initial fragmentation.
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The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution
The core mass function in 30Dor-10 is consistent with a Salpeter-like slope, implying that stellar IMF variations in extreme environments result from evolutionary processes rather than initial fragmentation.