activity
20052020
most citedGlobal Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario

366 citations · 708 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2020★ 42 cited

Density profile evolution during prestellar core collapse: Collapse starts at the large scale

Gilberto C. Gómez, Enrique Vázquez-Semadeni, Aina Palau

We study the gravitationally-dominated, accretion-driven evolution of a prestellar core. In our model, as the core's density increases, it remains immersed in a constant-density en…

astro-ph.GA2019★ 366 cited

Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario

Enrique Vázquez-Semadeni, Aina Palau, Javier Ballesteros-Paredes +2

We present a unified description of the scenario of Global Hierarchical Collapse and fragmentation (GHC) in molecular clouds (MCs), owing to the continuous decrease of the average…

astro-ph.GA2017★ 58 cited

MHD simulations of ram pressure stripping of a disk galaxy

Mariana Ramos-Martínez, Gilberto C. Gómez, Angeles Pérez-Villegas

The removal of the interstellar medium (ISM) of disk galaxies through ram pressure stripping (RPS) has been extensively studied in numerous simulations. Nevertheless, the role of m…

astro-ph.GA2016★ 42 cited

Energy budget of forming clumps in numerical simulations of collapsing clouds

Vianey Camacho, Enrique Vázquez-Semadeni, Javier Ballesteros-Paredes +3

We analyze the physical properties and energy balance of density enhancements in two SPH simulations of the formation, evolution, and collapse of giant molecular clouds. In the sim…

astro-ph.GA2015

The Galactic Branches as a Possible Evidence for Transient Spiral Arms

Angeles Pérez-Villegas, Gilberto C. Gómez, Bárbara Pichardo

With the use of a background Milky-Way-like potential model, we performed stellar orbital and magnetohydrodynamic (MHD) simulations. As a first experiment, we studied the gaseous r…

astro-ph.GA2014★ 11 cited

Analysis of the spiral structure in a simulated galaxy

Dolores Mata-Chávez, Gilberto C. Gómez, Ivânio Puerari

We analyze the spiral structure that results in a numerical simulation of a galactic disk with stellar and gaseous components evolving in a potential that includes an axisymmetric…