activity
20222024
most citedDiscovery of the elusive carbonic acid (HOCOOH) in space

54 citations · 212 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA2024

The GUAPOS project. V: The chemical ingredients of a massive stellar protocluster in the making

Á. López-Gallifa, V. M. Rivilla, M. T. Beltrán +9

Most stars, including the Sun, are born in rich stellar clusters containing massive stars. Therefore, the study of the chemical reservoir of massive star-forming regions is crucial…

astro-ph.GA2024

Physical Properties of the Southwest Outflow Streamer in the Starburst Galaxy NGC 253 with ALCHEMI

Min Bao, Nanase Harada, Kotaro Kohno +19

The physical properties of galactic molecular outflows are important as they could constrain outflow formation mechanisms. We study the properties of the southwest (SW) outflow str…

astro-ph.GA20241 cited

Interstellar detection of O-protonated carbonyl sulfide, HOCS+

Miguel Sanz-Novo, Víctor M. Rivilla, Izaskun Jiménez-Serra +12

We present the first detection in space of O-protonated carbonyl sulfide (\ch{HOCS+}), in the midst of an ultradeep molecular line survey toward the G+0.693-0.027 molecular cloud.…

astro-ph.GA2024

The ALCHEMI atlas: principal component analysis reveals starburst evolution in NGC 253

Nanase Harada, David S. Meier, Sergio Martín +24

Molecular lines are powerful diagnostics of the physical and chemical properties of the interstellar medium (ISM). These ISM properties, which affect future star formation, are exp…

astro-ph.GA202316 cited

Combined model for , , and spin-state chemistry in molecular clouds

O. Sipilä, L. Colzi, E. Roueff +3

We present a new gas-grain chemical model for the combined isotopic fractionation of carbon and nitrogen in molecular clouds, in which the isotope chemistry of carbon and nitrogen…

astro-ph.GA2023

The evolution of sulphur-bearing molecules in high-mass star-forming cores

F. Fontani, E. Roueff, L. Colzi +1

To understand the chemistry of sulphur (S) in the interstellar medium, models need to be tested by observations of S-bearing molecules in different physical conditions. We analyse…