activity
20062026
most citedAn Atomic and Molecular Study of the Interstellar Medium Around the SNR RCW 103

21 citations · 89 across the 23 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

26 papers · 1 filter

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.GA20251 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.GA20251 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.GA20247 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.GA2024

Understanding the chemistry of the young stellar object G29.862-0.0044

N. C. Martinez, S. Paron, D. Mast +3

In previous works, we have investigated the star-forming region G29.960.02 where the massive young stellar object (MYSO) G29.8620.0044 (hereafter G29) is embedded in a hot mo…

astro-ph.GA2024

Interstellar medium and star formation

S. Paron

The formation of stars, particularly the high-mass star formation, poses several still open questions. Nowadays, thanks to the most modern telescopes and instruments, we are able t…