66 citations · 132 across the 2 of their papers we have counts for
8 papers
Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
Ruby J. Wright, Claudia del P. Lagos, Chris Power +1
The inflow of cosmological gas onto haloes, while challenging to directly observe and quantify, plays a fundamental role in the baryon cycle of galaxies. Using the EAGLE suite of h…
The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
Camila A. Correa, Joop Schaye
We investigate the dependence of the local galaxy stellar-to-halo mass relation (SHMR) on galaxy morphology. We use data from the Sloan Digital Sky Survey DR7 with morphological cl…
Constraining Velocity-dependent Self-Interacting Dark Matter with the Milky Way's dwarf spheroidal galaxies
Camila A. Correa
The observed anti-correlation between the central dark matter (DM) densities of the bright Milky Way (MW) dwarf spheroidal galaxies (dSphs) and their orbital pericenter distances p…
The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
Florencia Collacchioni, Claudia D. P. Lagos, Peter D. Mitchell +4
We study the effect of the gas accretion rate () on the radial gas metallicity profile (RMP) of galaxies using the EAGLE cosmological hydrodynamic simulations, f…
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^{…
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…