activity
20102026
most citedThe HII region G35.673-00.847: another case of triggered star formation?

25 citations · 202 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2026

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

R. D. Taboada, N. C. Martinez, S. Paron +3

Astrochemical processes involving sulfur are not yet well understood because cosmic sulfur reservoirs and the production pathways of sulfur-bearing species remain elusive. Addressi…

astro-ph.GA2026

Exploring the chemical evolution in hot molecular cores

N. C. Martinez, S. Paron, M. E. Ortega +2

We present preliminary results of an extensive research project aimed at describing the physical and chemical conditions of hot molecular cores (HMCs). Using millimeter continuum a…

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.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.HE2023★ 2 cited

Radio and infrared study of the supernova remnant candidate HESS J1912+101

Laura Duvidovich, Alberto Petriella

Aims: We provide new insights into the gamma-ray emission from HESS J1912+101, a TeV supernova remnant candidate probably associated with the radio pulsar PSR J1913+1011. Methods:…