7 citations · 11 across the 7 of their papers we have counts for
7 papers
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…
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…
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…
Early phases of star formation: testing chemical tools
N. C. Martinez, S. Paron
The star forming processes strongly influence the ISM chemistry. Nowadays, there are available many high-quality databases at millimeter wavelengths. Using them, it is possible to…
Looking for evidence of high-mass star formation at core scale in a massive molecular clump
M. E. Ortega, N. C. Martinez, S. Paron +2
We present a comprehensive physical and chemical study of the fragmentation and star formation activity towards the massive clump AGAL G338.9188+0.5494 harbouring the extended gree…
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…
Studying a hot molecular core embedded in a photodissociation region
N. C. Martinez, M. B. Areal, S. Paron
At the first Galactic quadrant, at l=33.134, b=-0.091, an extended photodissociation region generated by an HII region complex lies. This region is related to abundant molecular ga…