The SEDIGISM survey: First Data Release and overview of the Galactic structure

F Schuller, JS Urquhart, T Csengeri… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic
Interstellar Medium) survey used the APEX telescope to map 84 deg2 of the Galactic plane …

Improved constraints from ultra-faint dwarf galaxies on primordial black holes as dark matter

J Stegmann, PR Capelo, E Bortolas… - Monthly Notices of the …, 2020 - academic.oup.com
Soon after the recent first ever detection of gravitational waves from merging black holes it
has been suggested that their origin is primordial. Appealingly, a sufficient number of …

Looking for evidence of high-mass star formation at core scale in a massive molecular clump

ME Ortega, NC Martinez, S Paron, A Marinelli… - Astronomy & …, 2023 - aanda.org
Context. High-mass stars are formed as a result of the fragmentation of massive molecular
clumps. However, what it is not clear is whether this fragmentation gives rise to stable …

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions–X. Chemical differentiation among the massive cores in G9. 62+ 0.19

Y Peng, T Liu, SL Qin, T Baug, HL Liu… - Monthly Notices of …, 2022 - academic.oup.com
Investigating the physical and chemical structure of massive star-forming regions is critical
for understanding the formation and early evolution of massive stars. We performed a …

Isocyanic acid (HNCO) in the hot molecular core G331. 512-0.103: observations and chemical modelling

CM Canelo, L Bronfman, E Mendoza… - Monthly Notices of …, 2021 - academic.oup.com
Isocyanic acid (HNCO) is a simple molecule with a potential to form prebiotic and complex
organic species. Using a spectral survey collected with the Atacama Pathfinder EXperiment …

Revisiting the massive star-forming complex RCW 122: New millimeter and submillimeter study

NU Duronea, L Bronfman, M Ortega, LA Suad… - Astronomy & …, 2024 - aanda.org
In this paper, we present a new multifrequency study of the giant star-forming complex RCW
122. We used molecular data obtained with the ASTE 10 m and the APEX 12 m telescopes …

LLAMA Millimeter and Submillimeter Observatory. Update on its Science Opportunities

M Fernandez-Lopez, P Benaglia, S Cichowolski… - arXiv preprint arXiv …, 2023 - arxiv.org
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 …

Early phases of star formation: testing chemical tools

NC Martinez, S Paron - Research in Astronomy and Astrophysics, 2023 - iopscience.iop.org
Star-forming processes strongly influence the ISM chemistry. Nowadays, many high-quality
databases are available at millimeter wavelengths. Using them, it is possible to carry out …

Observations and Chemical Modeling of the Isotopologues of Formaldehyde and the Cations of Formyl and Protonated Formaldehyde in the Hot Molecular Core G331 …

E Mendoza, M Carvajal, M Merello… - The Astrophysical …, 2023 - iopscience.iop.org
In the interstellar cold gas, the chemistry of formaldehyde (H 2 CO) can be essential to
explain the formation of complex organic molecules. On this matter, the massive and …

[HTML][HTML] The LLAMA Brazilian-Argentinian radiotelescope project: progress in Brazil and BRICS collaboration

JRD Lepine, Z Abraham, CGG CASTRO… - Anais da Academia …, 2021 - SciELO Brasil
We present briefly the LLAMA sub-mm radiotelescope, a joint project of Argentina and
Brazil, being mounted in the Andes, Argentina, at 4800 m altitude. Here we focus on the …