Meghan Hughes
0000-0002-0086-3813
4 papers found
Refreshing results…
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
The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations
The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
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