Robert A. Crain
www.astro.ljmu.ac.uk
0000-0001-6258-0344
147 papers found
Refreshing results…
The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
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 quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
A galaxy’s accretion history unveiled from its integrated spectrum
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
The abundance and physical properties of O vii and O viii X-ray absorption systems in the EAGLE simulations
The nature of submillimetre and highly star-forming galaxies in the EAGLE simulation
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
The E-MOSAICS project: tracing galaxy formation and assembly with the age–metallicity distribution of globular clusters
The diverse evolutionary pathways of post-starburst galaxies
Quasar Sightline and Galaxy Evolution (QSAGE) survey – I. The galaxy environment of O vi absorbers up to z = 1.4 around PKS 0232−04
The signal of decaying dark matter with hydrodynamical simulations
The gas fractions of dark matter haloes hosting simulated ∼L⋆ galaxies are governed by the feedback history of their black holes
The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
Galaxies with monstrous black holes in galaxy cluster environments
Evolution of the cold gas properties of simulated post-starburst galaxies
Calibrated, cosmological hydrodynamical simulations with variable IMFs III: spatially resolved properties and evolution
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