activity
20062026
most citedDense gas in the Galactic central molecular zone is warm and heated by turbulence

234 citations · 3.4k across the 79 of their papers we have counts for

collaborators

79 papers

astro-ph.GA2026

Detection of a four-carbon sugar in interstellar space

Izaskun Jimenez-Serra, Juan Garcia de la Concepcion, Herma M. Cuppen +19

Sugars are essential biomolecules, serving as metabolic fuels, nucleic acid backbone components, and structural or energy-storage polymers. A central question in origin-of-life res…

astro-ph.GA2026

Aromatic rings in the Central Molecular Zone: Benzonitrile

V. M. Rivilla, D. San Andrés, M. Sanz-Novo +12

In recent years, several aromatic molecules (benzene-based rings) have been detected in the cold molecular cloud TMC-1, with its CN-derivative, benzonitrile (c-CHCN), also…

astro-ph.GA2026

CII fine-structure line observations of the Sagittarius C Region in the Galaxy's Central Molecular Zone

DEnise Riquelme-Vasquez, Rolf Guesten, Mark R. Morris +7

Context. Sagittarius C (Sgr C) is a massive, relatively quiescent complex at the western edge of the Galaxy's Central Molecular Zone (CMZ). While the Sgr B2 region has been extensi…

astro-ph.GA2026★ 2 cited

Expanding the CHO Isomeric Interstellar Inventory: Discovery of Lactaldehyde and Methoxyacetaldehyde in G+0.693-0.027

M. Sanz-Novo, V. M. Rivilla, I. Jiménez-Serra +17

The tentative detection of 3-hydroxypropanal (HO(CH)C(O)H) toward the Galactic center molecular cloud G+0.693-0.027 prompts a systematic survey in this source aimed at dete…

astro-ph.IM2025

The Emergence of Prebiotic Chemistry in the ISM

Izaskun Jimenez-Serra, Giuliana Cosentino, Francisco Montenegro-Montes +22

Contrary to popular belief, the interstellar medium (ISM) is not empty; it is filled with atoms, dust particles, and molecules. Some of these molecules may have been the very build…

astro-ph.GA2025

The role of supernova remnants for the emergence of pre-biotic chemistry in molecular clouds

Giuliana Cosentino, Izaskun Jiménez-Serra, Laura Colzi +11

There is growing evidence that the Sun might have formed within a nebula impacted by at least one SNR. In this scenario, ejecta and shocks from SNRs may have provided the elements…