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20052022
most citedExploring the 13CO/C18O abundance ratio towards Galactic young stellar objects and HII regions

17 citations · 58 across the 10 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2022★ 5 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.GA2020★ 6 cited

Studying star-forming processes at core and clump scales: the case of the young stellar object G29.862-0.0044

M. B. Areal, S. Paron, C. Fariña +3

Massive molecular clumps fragment into cores where star formation takes place, hence star-forming studies should be done at different spatial scales. Using near-IR data obtained wi…

astro-ph.GA2019★ 7 cited

12CO and 13CO J=3-2 observations toward N11 in the Large Magellanic Cloud

M. Celis Peña, S. Paron, M. Rubio +2

After 30 Doradus, N11 is the second largest and brightest nebula in the LMC. This large nebula has several OB associations with bright nebulae at its surroundings. N11 was previous…

astro-ph.GA2018

Study of the molecular gas towards the N11 region in the Large Magellanic Cloud

M. Celis Peña, M. Rubio, S. Paron +1

We study three subregions in the HII region N11 which is located at the northeast side of the Large Magellanic Cloud (LMC). We used CO and CO J=3--2 data observed wit…

astro-ph.GA2017★ 17 cited

Exploring the 13CO/C18O abundance ratio towards Galactic young stellar objects and HII regions

M. B. Areal, S. Paron, Peña M. Celis +1

Determining molecular abundance ratios is important not only for the study of the Galactic chemistry but also because they are useful to estimate physical parameters in a large var…

astro-ph.GA2017★ 3 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…