activity
20202026
most citedPRODIGE -- Envelope to Disk with NOEMA III. The origin of complex organic molecule emission in SVS13A

14 citations · 69 across the 21 of their papers we have counts for

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Showing 2024Show all

7 papers · 1 filter

astro-ph.GA2024

Evolution of Chemistry in the envelope of HOt CorinoS (ECHOS) II. The puzzling chemistry of isomers as revealed by the HNCS/HSCN ratio

G. Esplugues, M. Rodríguez-Baras, D. Navarro-Almaida +8

The observational detection of some metastable isomers in the interstellar medium with abundances comparable to those of the most stable isomer, or even when the stable isomer is n…

astro-ph.GA2024★ 3 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS). X. Observational effects of turbulence on the chemistry of molecular clouds

L. Beitia-Antero, A. Fuente, D. Navarro-Almaida +12

(Abridged) We explore the chemistry of the most abundant C, O, S, and N bearing species in molecular clouds, in the context of the IRAM 30 m Large Programme Gas phase Elemental abu…

astro-ph.EP2024★ 10 cited

SO as shock tracer in protoplanetary disks: the AB Aurigae case

A. Dutrey, E. Chapillon, S. Guilloteau +9

{Sulfur Monoxide is known to be a good shock tracer in molecular clouds and protostar environments, but its abundance is difficult to reproduce even using state-of-the-art astroche…

astro-ph.IM2024

A fast neural emulator for interstellar chemistry

A. Asensio Ramos, C. Westendorp Plaza, D. Navarro-Almaida +3

Astrochemical models are important tools to interpret observations of molecular and atomic species in different environments. However, these models are time-consuming, precluding a…

astro-ph.GA2024★ 14 cited

PRODIGE -- Envelope to Disk with NOEMA III. The origin of complex organic molecule emission in SVS13A

T. -H. Hsieh, J. E. Pineda, D. M. Segura-Cox +18

Complex Organic Molecules (COMs) have been found toward low-mass protostars but the origins of the COM emission are still unclear. It can be associated with, for example, hot corin…

astro-ph.GA2024

Grain growth and its chemical impact in the first hydrostatic core phase

D. Navarro-Almaida, U. Lebreuilly, P. Hennebelle +8

The first hydrostatic core (FHSC) phase is a brief stage in the protostellar evolution that is difficult to detect. Our goal is to characterize the chemical evolution of gas and du…