From the top down and back up again: star cluster structure from hierarchical star formation.

@article{Grudic2018FromTT,
  title={From the top down and back up again: star cluster structure from hierarchical star formation.},
  author={M. Y. Grudi'c and D. Guszejnov and P. Hopkins and A. Lamberts and M. Boylan-Kolchin and N. Murray and Denise M. Schmitz},
  journal={Monthly notices of the Royal Astronomical Society},
  year={2018},
  volume={481 1},
  pages={
          688-702
        }
}
  • M. Y. Grudi'c, D. Guszejnov, +4 authors Denise M. Schmitz
  • Published 2018
  • Physics, Medicine
  • Monthly notices of the Royal Astronomical Society
  • Young massive star clusters spanning ~104-108M⊙ in mass have been observed to have similar surface brightness profiles. We show that recent hydrodynamical simulations of star cluster formation have also produced star clusters with this structure. We argue analytically that this type of mass distribution arises naturally in the relaxation from a hierarchically clustered distribution of stars into a monolithic star cluster through hierarchical merging. We show that initial profiles of finite… CONTINUE READING
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