127 papers found
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Calibrated, cosmological hydrodynamical simulations with variable IMFs III: spatially resolved properties and evolution
The evolution of the baryon fraction in haloes as a cause of scatter in the galaxy stellar mass in theeaglesimulation
Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
Calibrated, cosmological hydrodynamical simulations with variable IMFs – II. Correlations between the IMF and global galaxy properties
The rapid growth phase of supermassive black holes
The multiphase circumgalactic medium traced by low metal ions in EAGLE zoom simulations
The origin of the ‘blue tilt’ of globular cluster populations in the E-MOSAICS simulations
Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
SEAGLE – I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
The formation and assembly history of the Milky Way revealed by its globular cluster population
The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
The origin of diverse α-element abundances in galaxy discs
The impact of dark energy on galaxy formation. What does the future of our Universe hold?
Galaxy formation efficiency and the multiverse explanation of the cosmological constant with EAGLE simulations
Baryon Budget of the Hot Circumgalactic Medium of Massive Spiral Galaxies
The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons
SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
Globular cluster formation and evolution in the context of cosmological galaxy assembly: open questions
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