706 citations · 5.4k across the 58 of their papers we have counts for
55 papers
The origin of the stellar mass-size relation of satellite galaxies in the COLIBRE simulations
Bruno M. Celiz, Julio F. Navarro, Joop Schaye +9
We study the stellar mass-size relation of satellite galaxies in the COLIBRE suite of cosmological hydrodynamical simulations. Satellites deviate from the relation that holds for c…
Accreted stars and stellar haloes of simulated galaxies in TNG50
Bruno M. Celiz, Julio F. Navarro, Mario G. Abadi
We use the TNG50 cosmological hydrodynamic simulation to study the accreted stellar component and stellar haloes of isolated galaxies spanning a wide range of masses ($10^8<M_*/M_\…
Compact groups of galaxies in the TNG100 simulation
Bruno M. Celiz, José A. Benavides, Mario G. Abadi
Using the TNG100 cosmological simulation, we study the formation and evolution of compact groups of galaxies. Over a redshift range of , we identify thes…
Mass-morphology relation of TNG50 galaxies
Bruno M. Celiz, Julio F. Navarro, Mario G. Abadi +1
We used the cosmological hydrodynamical simulation TNG50 to study the galaxy mass-morphology relation, as measured by the rotational support of the stellar component of simulated g…
Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
Valeria A. Cristiani, Mario G. Abadi, Antonela Taverna +3
Galaxy formation is intrinsically connected to the distinct evolutionary processes of disk and spheroidal systems, which are the fundamental stellar components of galaxies. Underst…
The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
Silvio Rodriguez, Valeria A. Cristiani, Laura V. Sales +1
Disc dominated galaxies can be difficult to accommodate in a hierarchical formation scenario like CDM, where mergers are an important growth mechanism. However, observational ev…