most citedHigh-energy interstellar isomers: cis-N-methylformamide in the G+0.693-0.027 molecular cloud

1 citations · 2 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025

Piecing together formic acid isomerism in dark clouds. Detection of cis-formic acid in TMC-1 and astrochemical modeling

G. Molpeceres, M. Agúndez, M. Mallo +6

The presence of molecular isomers in interstellar environments has become a topic of growing interest within the astrochemical community. Contrary to predictions based on thermodyn…

astro-ph.GA20251 cited

High-energy interstellar isomers: cis-N-methylformamide in the G+0.693-0.027 molecular cloud

S. Zeng, V. M. Rivilla, M. Sanz-Novo +8

Isomerism in complex organic molecules provides key insights into the formation mechanisms and physical conditions of the interstellar medium (ISM). Among the CHNO isomers,…

astro-ph.GA2025

CO Depletion in Infrared Dark Clouds

G. Cosentino, J. C. Tan, C. Gainey +10

Infrared Dark Clouds (IRDCs) are cold, dense structures representative of the initial conditions of star formation. Many studies of IRDCs employ CO to investigate cloud dynamics. H…

astro-ph.GA2025

The GUAPOS project. VI: the chemical inventory of shocked gas

Á. López-Gallifa, V. M. Rivilla, M. T. Beltrán +8

The study of the chemical composition of star-forming regions is key to understanding the chemical ingredients available during the formation of planetary systems. Because the chem…

astro-ph.GA2025

Rotational Spectroscopy and Tentative Interstellar Detection of 3-Hydroxypropanal (HOCHCHCHO) in the G+0.693-0.027 Molecular Cloud

Zachary T. P. Fried, Roman A. Motiyenko, Miguel Sanz-Novo +12

We synthesized the astrochemically relevant molecule 3-hydroxypropanal (HOCHCHCHO) and subsequently measured and analyzed its rotational spectrum in several frequency regio…

astro-ph.GA2025

Chemical templates of the Central Molecular Zone. Shock and protostellar object signatures under Galactic Center conditions

Katarzyna M. Dutkowska, Gijs Vermariën, Serena Viti +21

(Abridged) The Central Molecular Zone (CMZ) of the Milky Way exhibits extreme conditions, including high gas densities, elevated temperatures, enhanced cosmic-ray ionization rates,…