activity
20002020
most citedResults of the ESO-SEST Key Programme on CO in the Magellanic Clouds X. CO emission from star formation regions in LMC and SMC

66 citations · 270 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2020★ 11 cited

Resolved star formation in the metal poor star-forming region Magellanic Bridge C

V. M. Kalari, M. Rubio, H. P. Saldaño +1

Magellanic Bridge C (MB-C) is a metal-poor (1/5 ) low-density star-forming region located 59 kpc away in the Magellanic Bridge, offering a resolved view of the sta…

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★ 1 cited

Millimeter and far-IR study of the IRCD SDC 341.232-0.268

M. M. Vazzano, C. E. Cappa, V. Firpo +3

We analyze the molecular gas and dust associated with the infrared dark cloud SDC 341.232-0.268 in order to investigate the characteristics and parameters of the gas, determine the…

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.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…

astro-ph.GA2017★ 7 cited

Dust emission at 8-mic and 24-mic as Diagnostics of HII Region Radiative Transfer

M. S. Oey, J. Lopez-Hernandez, J. A. Kellar +10

We use the Spitzer SAGE survey of the Magellanic Clouds to evaluate the relationship between the 8-mic PAH emission, 24-mic hot dust emission, and HII region radiative transfer. We…