activity
20162024
most citedComparing binary systems from rotating parent gas structures with different total masses

5 citations · 6 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2024

Using Cartesian slice plots of a cosmological simulation as input of a convolutional neural network

Guillermo Arreaga-Garcia

Using a uniform partitioning of cubic cells, we cover the total volume of a CDM cosmological simulation based on particles. We define a visualisation cell as a spatial extension…

astro-ph.CO2021

Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity

Guillermo Arreaga-Garcia

By means of identical cubic elements, we generate a partition of a volume in which a particle-based cosmological simulation is carried out. In each cubic element, we determine the…

astro-ph.GA2020

A thick-disk galaxy model and simulations of equal-mass galaxy pair collisions

Guillermo Arreaga-Garcia

We implement a numerical model reported in the literature to simulate the evolution of a galaxy composed of four matter components, such as: a dark-matter halo; a rotating disk of…

astro-ph.SR2019

The effects of a compressive velocity pulse on a collapsing turbulent clump

G. Arreaga-Garcia

High-resolution hydrodynamical simulations are presented to follow the gravitational collapse of a uniform turbulent clump, upon which a purely radial compressive velocity pulse is…

astro-ph.SR2018

The extreme initial kinetic energy allowed by a collapsing turbulent core

Guillermo Arreaga-Garcia

We present high-resolution hydrodynamical simulations aimed at following the gravitational collapse of a gas core, in which a turbulent spectrum of velocity is implemented only ini…

astro-ph.SR20171 cited

The effects on a core collapse of changes in the number and size of turbulent modes of velocity

Guillermo Arreaga-Garcia

We consider 28 particle-based simulations aimed at comparing the gravitational collapse of a spherically symmetric, uniform gas core in which two extreme types of turbulent spectra…