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Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
James W. Trayford, Joop Schaye
We explore scaling relations between the physical properties of spatially resolved regions within the galaxies that emerge in the Evolution and Assembly of GaLaxies and their Envir…
The origin of the red sequence galaxy population in the EAGLE simulation
Camila A. Correa, Joop Schaye, James W. Trayford
We investigate the evolution in colour and morphology of the progenitors of red-sequence galaxies in the EAGLE cosmological hydrodynamical simulation. We quantify colours with $u^{…
Quenching timescales of galaxies in the EAGLE simulations
Ruby J. Wright, Claudia del P. Lagos, Luke J. M. Davies +3
We use the \eagle\ simulations to study the connection between the quenching timescale, , and the physical mechanisms that transform star-forming galaxies into passive g…
Ring Galaxies in the EAGLE Hydrodynamical Simulations
Ahmed Elagali, Claudia D. P. Lagos, O. Ivy Wong +5
We study the formation and evolution of ring galaxies in the Evolution and Assembly of GaLaxies and their Environments (EAGLE) simulations. We use the largest reference model Ref-L…
The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
James W. Trayford, Carlos S. Frenk, Tom Theuns +2
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, morphologies are not static, but rather evolve as the growth of structure procee…