activity
20142023
most citedDetailed study of SNR G306.3-0.9 using XMM-Newton and Chandra observations

7 citations · 19 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2023

An analysis of the isomers HCN and HNC in the evolution of high-mass star-forming regions

N. C. Martinez, S. Paron

The study of molecules and their chemistry in star-forming regions is fundamental to understand the physical process occurring in such regions. The HCN and HNC J=1-0 emissions were…

astro-ph.GA20225 cited

Studying a precessing jet of a massive young stellar object within a chemically rich region

S. Paron, D. Mast, C. Fariña +4

In addition to the large surveys and catalogs of massive young stellar objects and outflows, dedicated studies of particular sources, in which high-angular observations (mainly at…

astro-ph.GA20211 cited

Unveiling the substructure of the massive clump AGAL G035.133000.7450

M. E. Ortega, A. Marinelli, N. L. Isequilla +1

It is known that massive stars form as result of the fragmentation of molecular clumps. However, what is not clear is whether this fragmentation gives rise to cores massive enough…

astro-ph.GA20173 cited

Study of the molecular and ionized gas in a possible precursor of an ultra-compact HII region

M. E. Ortega, S. Paron, E. Giacani +3

We study the molecular and the ionized gas in a possible precursor of an UC HII region to contribute to the understanding of how high-mass stars build-up their masses once they hav…

astro-ph.GA20143 cited

Discovering a misaligned CO outflow related to the red MSX source G034.5964-01.0292

S. Paron, M. E. Ortega, A. Petriella +1

The red MSX source G034.5964-01.0292 (MSXG34), catalogued as a massive YSO, was observed in molecular lines with the aim of discover and study molecular outflows. We mapped a regio…