4 papers
From atoms to stars: Modelling formation and its impact on galactic evolution
E. Lozano, C. Scannapieco, S. E. Nuza +2
We present a sub-grid model for star formation in galaxy simulations, incorporating molecular hydrogen () production via dust grain condensation and its destruction t…
Kinematic patterns of the enriched gas phase in the Local Group {\sc Hestia} simulations
L. Biaus, S. E. Nuza, C. Scannapieco +2
Observations of intergalactic absorbers in the Local Group suggest the existence of a velocity dipole in the general barycentre--antibarycentre direction which can be interpreted a…
The distribution of metals in simulated Milky Way-mass galaxies
Federico G. Iza, Sebastián E. Nuza, Cecilia Scannapieco +2
Galaxies form due to the continuous accretion of gaseous material towards the centre of dark matter haloes, which gives rise to stellar discs once the gas reaches high density. Ana…
Enhanced sub-resolution star formation models in cosmological simulations
Ezequiel Lozano, Cecilia Scannapieco, Sebastián E. Nuza +3
One of the crucial components in simulating the growth and evolution of galaxies within a cosmological framework is the modeling of star formation (SF) and its corresponding feedba…