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Meghan E. Hughes

Liverpool John Moores University

19

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258

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Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations.

2021 arXiv: Astrophysics of Galaxies
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What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies

2021 Monthly Notices of the Royal Astronomical Society
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What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies.

2021 arXiv: Astrophysics of Galaxies
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The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way

2021 Monthly Notices of the Royal Astronomical Society
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Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS

2020 Monthly Notices of the Royal Astronomical Society
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Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations.

2020 arXiv: Astrophysics of Galaxies
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Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS

2020 arXiv: Astrophysics of Galaxies
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Kraken reveals itself -- the merger history of the Milky Way reconstructed with the E-MOSAICS simulations.

2020 arXiv: Astrophysics of Galaxies
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The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way

2020 arXiv: Astrophysics of Galaxies
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The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations

2020 Monthly Notices of the Royal Astronomical Society
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