25 citations · 202 across the 24 of their papers we have counts for
16 papers · 1 filter
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…
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…
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…
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…
The molecular environment of the pillar-like features in the HII region G46.5-0.2
S. Paron, M. Celis Peña, M. E. Ortega +3
At the interface of HII regions and molecular gas peculiar structures appear, some of them with pillar-like shapes. Understanding their origin is important for characterizing trigg…
Radio and X-ray properties of the source G29.37+0.1 linked to HESS J1844-030
G. Castelletti, L. Supan, A. Petriella +2
Using observations carried out with the GMRT, we performed high-quality full-synthesis imaging at 610 MHz of the source G29.37+0.1, which is an as-yet-unclassified object linked to…
HII region G46.5-0.2: the interplay between ionizing radiation, molecular gas and star formation
S. Paron, M. E. Ortega, G. Dubner +8
HII regions are particularly interesting because they can generate dense layers of gas and dust, elongated columns or pillars of gas pointing towards the ionizing sources, and come…
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…
An X-ray study of the supernova remnant G20.0-0.2 and its surroundings
Alberto Petriella, Sergio Paron, Elsa Giacani
Aims: We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high energy counterpart of the radio nebula and to find evidence of interaction between…
The molecular clump towards the eastern border of SNR G18.8+0.3
S. Paron, M. E. Ortega, A. Petriella +3
The eastern border of the SNR G18.8+0.3, close to an HII regions complex, is a very interesting region to study the molecular gas that it is probably in contact with the SNR shock…
Study of the luminous blue variable star candidate G26.47+0.02 and its environment
S. Paron, J. A. Combi, A. Petriella +1
The luminous blue variable (LBV) stars are peculiar very massive stars. The study of these stellar objects and their surroundings is important for understanding the evolution of ma…
Study of the dense molecular gas surrounding the "Extended Green Object" G35.03+0.35
S. Paron, M. E. Ortega, A. Petriella +3
We present the results of a new study of the molecular gas associated with the "extended green object" (EGO) G35.03+0.35. This object, very likely a massive young stellar object, i…
The HII region G35.673-00.847: another case of triggered star formation?
S. Paron, A. Petriella, M. E. Ortega
As part of a systematic study that we are performing with the aim to increase the observational evidence of triggered star formation in the surroundings of HII regions, we analyze…
The environment of the infrared dust bubble N65: a mutiwavelength study
A. Petriella, S. A. Paron, E. B. Giacani
AIMS: We investigate the environment of the infrared dust bubble N65 and search for evidence of triggered star formation in its surroundings. METHODS: We performed a multiwavelengt…