activity
20182022
most citedCyano radical emission at small spatial scales towards massive protostars

9 citations · 32 across the 9 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2022

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…

astro-ph.GA20219 cited

Cyano radical emission at small spatial scales towards massive protostars

S. Paron, M. E. Ortega, A. Marinelli +2

The cyano radical (CN), one of the first detected interstellar molecular species, is a key molecule in many astrochemical chains. Particularly, it is detected towards molecular cor…

astro-ph.GA20213 cited

Studying the interstellar medium to look for relics of triggered star formation among stellar clusters

S. Paron, A. Granada, M. B. Areal

Evidence of triggered star formation at large spatial scales involving stellar clusters is scarce. We investigate a Galactic region (l=130.0, b=0.35) populated by several open stel…

astro-ph.GA2021

Multiple molecular outflows and fragmentation in the IRDC core G34.43+00.24 MM1

N. L. Isequilla, M. E. Ortega, M. B. Areal +1

The fragmentation of a molecular cloud that leads to the formation of high-mass stars occurs on a hierarchy of different spatial scales. The large molecular clouds harbour massive…

astro-ph.GA20206 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.GA20202 cited

Three generations of stars: a possible case of triggered star formation

M. B. Areal, A. Buccino, S. Paron +2

Evidence for triggered star formation linking three generations of stars is difficult to assemble, as it requires convincingly associating evolved massive stars with Hii regions th…