14 papers found
Refreshing results…
Kraken reveals itself -- the merger history of the Milky Way reconstructed with the E-MOSAICS simulations
Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
The [α/Fe]–[Fe/H] relation in the E-MOSAICS simulations: its connection to the birth place of globular clusters and the fraction of globular cluster field stars in the bulge
Young star cluster populations in the E-MOSAICS simulations
The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations
A model for the minimum mass of bound stellar clusters and its dependence on the galactic environment
The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
Formation histories of stars, clusters, and globular clusters in the E-MOSAICS simulations
A systematic analysis of star cluster disruption by tidal shocks – I. Controlled N-body simulations and a new theoretical model
The origin of metal-poor and metal-rich globular clusters in E-MOSAICS
Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
The origin of the ‘blue tilt’ of globular cluster populations in the E-MOSAICS simulations
The formation and assembly history of the Milky Way revealed by its globular cluster population
A unified model for the maximum mass scales of molecular clouds, stellar clusters and high-redshift clumps
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