activity
20192025
most citedModelling the prompt optical emission of GRB 180325A: the evolution of a spike from the optical to gamma-rays

13 citations · 17 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Gravitationally Induced Explosive Outflows

Pedro Ruben Rivera-Ortiz, Ary Rodríguez-González, Jorge Cantó +4

Over the past decade, there has been a significant increase in the reporting of extensive and luminous star-forming regions associated with explosive outflows. Nevertheless, there…

astro-ph.GA2022★ 4 cited

Modelling the CO streamers in the explosive ejection of Orion BN/KL region

Ary Rodríguez-González, Pedro Ruben Rivera-Ortiz, Antonio Castellanos-Ramírez +5

We present reactive gasdynamic, axisymmetric simulations of dense, high velocity clumps for modelling the CO streamers observed in Orion BN/KL. We have considered 15 chemical speci…

astro-ph.GA2021

Explosive ejections generated by gravitational interactions

Pedro Ruben Rivera-Ortiz, Ary Rodríguez-González, Jorge Cantó +1

During the fragmentation and collapse of a molecular cloud, it is expected to have close encounters between (proto)stellar objects that can lead to the ejection of a fraction of th…

astro-ph.HE2020★ 13 cited

Modelling the prompt optical emission of GRB 180325A: the evolution of a spike from the optical to gamma-rays

Rosa L. Becerra, Fabio De Colle, Jorge Cantó +20

The transition from prompt to the afterglow emission is one of the most exciting and least understood phases in gamma-ray bursts (GRBs). Correlations among optical, X-ray and gamma…

astro-ph.SR2019

The initial physical conditions of the Orion BN/KL fingers

Pedro Ruben Rivera-Ortiz, Ary Rodríguez-González, Liliana Hernández-Martínez +2

Orion BN/KL is an example of a poorly understood phenomena in star forming regions involving the close encounter of young stellar objects. The explosive structure, the great variet…

astro-ph.GA2019

The motion of a losing mass plasmon

Pedro Ruben Rivera-Ortiz, Ary Rodríguez-González, Liliana Hernández-Martínez +1

The interaction of a high velocity clump of gas has been described by the plasmon model, which considers balance between ram pressure and the internal stratified structure of the d…