Salpeter-like slope can often describe the stellar initial mass function, but its universality and the link with core mass function are unknown. Here, the authors show high resolution observations of three massive clumps in 30Dor-10 region, which are consistent with Salpeter-like slope, supporting an evolving and multi-scale star formation scenario.
- Alessio Traficante
- María J. Jiménez-Donaire
- Juan D. Soler
