about
P185
Properties of galaxies reproduced by a hydrodynamic simulation.Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the UniverseThe illustris simulation: Public data releaseA model for cosmological simulations of galaxy formation physicsFirst results from the IllustrisTNG simulations: matter and galaxy clusteringThe fraction of dark matter within galaxies from the IllustrisTNG simulationsFormation of a Malin 1 analogue in IllustrisTNG by stimulated accretionSupermassive black holes and their feedback effects in the IllustrisTNG simulationFirst results from the IllustrisTNG simulations: radio haloes and magnetic fieldsA census of cool-core galaxy clusters in IllustrisTNGChemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulationsFirst results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europiumSimilar star formation rate and metallicity variability time-scales drive the fundamental metallicity relationThe abundance, distribution, and physical nature of highly ionized oxygen O vi, O vii, and O viii in IllustrisTNGFirst results from the IllustrisTNG simulations: the galaxy colour bimodalityFirst results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxiesModelling galactic conformity with the colour–halo age relation in the Illustris simulationAn analysis of the evolving comoving number density of galaxies in hydrodynamical simulationsGalaxy morphology and star formation in the Illustris Simulation atz = 0Hydrogen reionization in the Illustris universeThe Illustris simulation: the evolving population of black holes across cosmic timeThe formation of massive, compact galaxies at z = 2 in the Illustris simulationThe merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical modelsSynthetic galaxy images and spectra from the Illustris simulationThe impact of feedback on cosmological gas accretionThe impact of galactic feedback on the circumgalactic mediumThe star formation main sequence and stellar mass assembly of galaxies in the Illustris simulationThe colours of satellite galaxies in the Illustris simulationDamped Lyman α absorbers as a probe of stellar feedbackIntroducing the Illustris project: the evolution of galaxy populations across cosmic timeHalo mass and assembly history exposed in the faint outskirts: the stellar and dark matter haloes of Illustris galaxiesGalaxy mergers on a moving mesh: a comparison with smoothed particle hydrodynamicsA model for cosmological simulations of galaxy formation physics: multi-epoch validationMoving-mesh cosmology: properties of gas discsGalaxy mergers moulding the circum-galactic medium – I. The impact of a major mergerThe incidence of low-metallicity lyman-limit systems at z ~ 3.5: implications for the cold-flow hypothesis of baryonic accretionAn integral field study of abundance gradients in nearby luminous infrared galaxiesSimulating galactic dust grain evolution on a moving meshOn the assembly of dwarf galaxies in clusters and their efficient formation of globular clustersOn the cosmic evolution of Fe/Mg in QSO absorption line systems
P50
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P50
description
hulumtues
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Paul Torrey
@ast
Paul Torrey
@en
Paul Torrey
@es
Paul Torrey
@nl
Paul Torrey
@sl
type
label
Paul Torrey
@ast
Paul Torrey
@en
Paul Torrey
@es
Paul Torrey
@nl
Paul Torrey
@sl
prefLabel
Paul Torrey
@ast
Paul Torrey
@en
Paul Torrey
@es
Paul Torrey
@nl
Paul Torrey
@sl
P106
P184
P21
P31
P496
0000-0002-5653-0786