The galactocentric radius dependent upper mass limit of young star clusters: stochastic star formation ruled out

@article{PflammAltenburg2013TheGR,
  title={The galactocentric radius dependent upper mass limit of young star clusters: stochastic star formation ruled out},
  author={Jan Pflamm-Altenburg and Rosa A. Gonzalez-L'opezlira and Pavel Kroupa},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={435},
  pages={2604-2609}
}
It is widely accepted that the distribution function of the masses of young star clusters is universal and can be purely interpreted as a probability density distribution function with a constant upper mass limit. As a result of this picture the masses of the mostmassive objects are exclusively determined by the size of the sample. Here we show, with very high confidence, that the masses of the most-massive young star clusters in M33 decrease with increasing galactocentric radius in… 

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