18 citations · 36 across the 8 of their papers we have counts for
8 papers
HCN, HCN, and HNC in molecular cores evolving towards star-forming regions
R. D. Taboada, S. Paron, M. E. Ortega +1
As a work in progress, results from a chemical and physical analysis of molecular cores in early evolutionary stages concerning star formation are presented. Using archival data fr…
Dense clumps survive in the vicinity of R136 in 30 Doradus
M. T. Valdivia-Mena, M. Rubio, V. M. Kalari +5
Context: The young massive cluster R136 at the center of 30 Doradus (30 Dor) in the Large Magellanic Cloud (LMC) generates a cavity in the surrounding molecular cloud. However, the…
LLAMA Millimeter and Submillimeter Observatory. Update on its Science Opportunities
M. Fernandez-Lopez, P. Benaglia, S. Cichowolski +11
The Large Latin American Millimeter Array (LLAMA for short) is a joint scientific and technological undertaking of Argentina and Brazil whose goal is to install and to operate an o…
SuperCAM CO(3-2) APEX survey at 6 pc resolution in the Small Magellanic Clouds
H. P. Saldaño, M. Rubio, A. D. Bolatto +9
We present the CO(3-2) APEX survey at 6 pc resolution of the bar of the SMC. We aboard the CO analysis in the SMC-Bar comparing the CO(3-2) survey with that of the CO(2-1) of simil…
CO(2-1) Survey at 9 parsec resolution in the SMC
H. P. Saldaño, M. Rubio, A. D. Bolatto +3
The Small Magellanic Cloud (SMC) is the closest low-metallicity galaxy to the Milky Way where the dynamical state of molecular clouds can be analyzed. We present a CO(2-1) survey a…
High-resolution images of two wiggling stellar jets, MHO 1502 and MHO 2147, obtained with GSAOI+GeMS
L. V. Ferrero, G. Günthardt, L. García +3
We investigated the possible cause-effect relation between the wiggling shape of two stellar jets, MHO 1502 and MHO 2147, and the potential binarity of the respective driving stars…
Multifrequency study of HH 137 and HH 138: Discovering new knots and molecular outflows with Gemini and APEX
Leticia V. Ferrero, Cristina E. Cappa, Hugo P. Saldaño +3
We present a multi-wavelength study of two HH objects (137 and 138) that may be associated. We use Gemini H (2.12 m) and K (2.2 m) images, as well as APEX molecular line…
Molecular gas in the star-forming region IRAS 08589-4714
Hugo P. Saldaño, J. Vásquez, C. E. Cappa +3
We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. We observed the CO(3-2), ^{13}CO(3-2), C^{18}O(3-2), HCO+(3-2), and H…