Primordial mass segregation of star clusters with primordial binaries

@article{Pavlik2020PrimordialMS,
  title={Primordial mass segregation of star clusters with primordial binaries},
  author={V'aclav Pavl'ik},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
Context. Observations of young star-forming regions suggest that star clusters are born completely mass segregated. These initial conditions are, however, gradually lost as the star cluster evolves dynamically. For star clusters with single stars only and a canonical initial mass function, it has been suggested that traces of these initial conditions vanish at a time τv between 3 and 3.5 trh (initial half-mass relaxation times). Aims. Since a significant fraction of stars are observed in binary… 

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