activity
20212026
most citedKinematics of the Local Group gas and galaxies in the Hestia simulations

4 citations · 4 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Probing the kinematics of the Local Group with chemically enriched gas in the Hestia simulations

L. Biaus, S. E. Nuza, C. Scannapieco +4

We present a study of the gas kinematics within the Hestia project, a state-of-the-art set of simulations of the Local Group, with a particular focus on the velocity patterns of di…

astro-ph.GA2025

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…

astro-ph.GA2025

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…

astro-ph.GA2025

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…

astro-ph.GA20224 cited

Kinematics of the Local Group gas and galaxies in the Hestia simulations

Luis Biaus, Sebastián E. Nuza, Philipp Richter +8

We investigate the kinematic properties of gas and galaxies in the Local Group (LG) using high-resolution simulations performed by the {\sc Hestia} (High-resolution Environmental S…

astro-ph.GA2021

Chemical abundance patterns in Local Group galaxies within cosmological simulations

L. Biaus, C. Scannapieco, S. E. Nuza

In the context of the concordance cosmology, structure formation in the Universe is the result of the amplification, by gravitational effects, of small perturbations in the primeva…