Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster

@article{Kroupa2018EvidenceFF,
  title={Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster},
  author={Pavel Kroupa and Tereza Jeř{\'a}bkov{\'a} and Frantivsek Dinnbier and Giacomo Beccari and Zhiqiang Yan},
  journal={Astronomy and Astrophysics},
  year={2018},
  volume={612}
}
(abridged) A scenario for the formation of multiple co-eval populations separated in age by about 1 Myr in very young clusters (VYCs, ages less than 10 Myr) and with masses in the range 600-20000 Msun is outlined. It rests upon a converging inflow of molecular gas building up a first population of pre-main sequence stars. The associated just-formed O stars ionise the inflow and suppress star formation in the embedded cluster. However, they typically eject each other out of the embedded cluster… 

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