Formation of globular cluster candidates in merging proto-galaxies at high redshift: A view from the FIRE cosmological simulations

Ji Hoon Kim*, Xiangcheng Ma, Michael Y. Grudić, Philip F. Hopkins, Christopher C. Hayward, Andrew Wetzel, Claude André Faucher-Giguère, Dušan Kereš, Shea Garrison-Kimmel, Norman Murray

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

39 Scopus citations


Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the FIRE project, with explicit treatments of star formation and stellar feedback in the interstellar medium, we investigate the formation of star clusters and examine one of the formation hypotheses of present-day metal-poor globular clusters. We find that frequent mergers in high-redshift proto-galaxies could provide a fertile environment to produce long-lasting bound star clusters. The violent merger event disturbs the gravitational potential and pushes a large gas mass of ≳ 105-6M collectively to high density, at which point it rapidly turns into stars before stellar feedback can stop star formation. The high dynamic range of the reported simulation is critical in realizing such dense star-forming clouds with a small dynamical time-scale, tff ≲ 3 Myr, shorter than most stellar feedback time-scales. Our simulation then allows us to trace how clusters could become virialized and tightly bound to survive for up to ~420 Myr till the end of the simulation. Because the cluster's tightly bound core was formed in one short burst, and the nearby older stars originally grouped with the cluster tend to be preferentially removed, at the end of the simulation the cluster has a small age spread.

Original languageEnglish (US)
Pages (from-to)4232-4244
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Issue number3
StatePublished - Mar 1 2018


  • Cosmology: theory
  • Galaxies: formation
  • Galaxies: kinematics and dynamics
  • Galaxies: star clusters: general
  • Globular clusters: general
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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