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Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations

Reina-Campos, M, Kruijssen, JMD, Pfeffer, JL, Bastian, N and Crain, RA (2019) Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations. Monthly Notices of the Royal Astronomical Society, 486 (4). pp. 5838-5852. ISSN 0035-8711

1905.02217v1.pdf - Accepted Version

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The formation histories of globular clusters (GCs) are a key diagnostic for understanding their relation to the evolution of the Universe through cosmic time. We use the suite of 25 cosmological zoom-in simulations of present-day Milky Way-mass galaxies from the E-MOSAICS project to study the formation histories of stars, clusters, and GCs, and how these are affected by the environmental dependence of the cluster formation physics. We find that the median lookback time of GC formation in these galaxies is ${\sim}10.73~$Gyr ($z=2.1$), roughly $2.5~$Gyr earlier than that of the field stars (${\sim}8.34~$Gyr or $z=1.1$). The epoch of peak GC formation is mainly determined by the time evolution of the maximum cluster mass, which depends on the galactic environment and largely increases with the gas pressure. Different metallicity subpopulations of stars, clusters and GCs present overlapping formation histories, implying that star and cluster formation represent continuous processes. The metal-poor GCs ($-2.5<[\rm Fe/H]<-1.5$) of our galaxies are older than the metal-rich GC subpopulation ($-1.0<[\rm Fe/H]<-0.5$), forming $12.13~$Gyr and $10.15~$Gyr ago ($z=3.7$ and $z=1.8$), respectively. The median ages of GCs are found to decrease gradually with increasing metallicity, which suggests different GC metallicity subpopulations do not form independently and their spatial and kinematic distributions are the result of their evolution in the context of hierarchical galaxy formation and evolution. We predict that proto-GC formation is most prevalent at $2\lesssim z \lesssim 3$, which could be tested with observations of lensed galaxies using JWST.

Item Type: Article
Additional Information: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Marta Reina-Campos, J M Diederik Kruijssen, Joel L Pfeffer, Nate Bastian, Robert A Crain, Formation histories of stars, clusters, and globular clusters in the E-MOSAICS simulations, Monthly Notices of the Royal Astronomical Society, Volume 486, Issue 4, July 2019, Pages 5838–5852 is available online at: https://doi.org/10.1093/mnras/stz1236
Uncontrolled Keywords: 0201 Astronomical and Space Sciences
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 21 Jun 2019 15:00
Last Modified: 04 Sep 2021 09:15
DOI or Identification number: 10.1093/mnras/stz1236
URI: https://researchonline.ljmu.ac.uk/id/eprint/10923

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