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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Across seven molecular clouds the integrated filament linear density function follows a power law with slope 1.30-1.34, matching the Salpeter IMF slope of 1.35.
citing papers explorer
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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.
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A Salpeter-like filament linear density function across nearby molecular clouds
Across seven molecular clouds the integrated filament linear density function follows a power law with slope 1.30-1.34, matching the Salpeter IMF slope of 1.35.