activity
20082026
most citedA joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946

74 citations · 450 across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2026

Simple cyanides and formylium ions isotopologues in early star-forming molecular cores

R. D. Taboada, S. Paron, N. C. Martinez +1

Understanding the chemistry related to the early stages of star formation is of great importance, as it is linked to the beginnings of the most complex chemistry in the interstella…

astro-ph.GA2026

Characterization of molecular outflows at core-scale in the massive clump AGAL G345.0029-0.224

E. Cohen Arazi, M. E. Ortega, S. Paron +3

High-mass stars, with their powerful winds and intense radiation fields, are fundamental in regulating galactic dynamics and evolution; however, despite their great relevance, the…

astro-ph.GA2025★ 1 cited

Unveiling the collision between molecular outflows: observational evidence and hydrodynamic simulations

E. Cohen Arazi, P. F. Velázquez, M. E. Ortega +5

We present an unexplored scenario for interpreting the outflows in the EGO G338.92+0.55 (b) region (hereafter, EGO G338). Within this framework, we investigate the hypothesis that…

astro-ph.GA2025★ 1 cited

Revisiting G29.862-0.0044: a jet cavity disrupted by an outflow in a likely young stellar object wide binary system

S. Paron, N. C. Martinez, M. E. Ortega +4

A few years ago, we investigated MYSO G29.862-0.0044 (YSO-G29), an intriguing star-forming region at a distance of 6.2 kpc. Although the typical disc-jet scenario was proposed to e…

astro-ph.GA2024★ 7 cited

Sulfur-bearing molecules in a sample of early star-forming cores

N. C. Martinez, S. Paron, M. E. Ortega +5

The sulfur content in dense molecular regions of the interstellar medium is highly depleted in comparison to diffuse clouds. The reason of this phenomenon is unclear, thus it is ne…

astro-ph.HE2024

A comprehensive analysis toward the Fermi-LAT source 4FGL J1846.9-0227: Jets of a proto-planetary nebula producing gamma-rays?

M. E. Ortega, A. Petriella, S. Paron

Most of the -ray sources in the Fermi-LAT 14-year Source Catalogue are associated with pulsars and blazars. However, unveiling the nature of the still unassociated -ray sourc…