No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud

@article{Grijs2013NoCE,
  title={No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud},
  author={Richard de Grijs and S. P. Goodwin and Peter Anders Kavli Institute for Astronomy and Astrophysics and Peking University and Beijing and China. and Department of Physics Astronomy and Dep. of Physics and Astronomy and University of Sheffield and Sheffield and UK. and Key Laboratory of Optical Astronomy and National Astronomical Observatories and Chinese Academy of Sciences},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={436},
  pages={136-149}
}
Whether or not the rich star cluster population in the Large Magellanic Cloud (LMC) is affected by significant disruption during the first few × 108 yr of its evolution is an open question and the subject of significant current debate. Here, we revisit the problem, adopting a homogeneous data set of broad-band imaging observations. We base our analysis mainly on two sets of self-consistently determined LMC cluster ages and masses, one using standard modelling and one which takes into account… 

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