activity
20062026
most citedAn Ice Age JWST inventory of dense molecular cloud ices

363 citations · 3.3k across the 50 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2025★ 12 cited

Molecular Mobility of Extraterrestrial Ices: Surface Diffusion in Astrochemistry and Planetary Science

N. F. W. Ligterink, C. Walsh, H. M. Cuppen +12

Molecules are ubiquitous in space. They are necessary component in the creation of habitable planetary systems and can provide the basic building blocks of life. Solid-state proces…

astro-ph.SR2020★ 76 cited

Formation of COMs through CO hydrogenation on interstellar grains

M. A. J. Simons, T. Lamberts, H. M. Cuppen

Glycoaldehyde, ethylene glycol, and methyl formate are complex organic molecules that have been observed in dark molecular clouds. Because there is no efficient gas-phase route to…

astro-ph.SR2015★ 6 cited

Low-temperature chemistry between water and hydroxyl radicals: H/D isotopic effects

T. Lamberts, G. Fedoseev, F. Puletti +3

Sets of systematic laboratory experiments are presented -- combining Ultra High Vacuum cryogenic and plasma-line deposition techniques -- that allow us to compare H/D isotopic effe…

astro-ph.SR2010★ 147 cited

Water formation at low temperatures by surface O2 hydrogenation II: the reaction network

H. M. Cuppen, S. Ioppolo, C. Romanzin +1

Water is abundantly present in the Universe. It is the main component of interstellar ice mantles and a key ingredient for life. Water in space is mainly formed through surface rea…

astro-ph.SR2010★ 114 cited

Water formation at low temperatures by surface O2 hydrogenation I: characterization of ice penetration

S. Ioppolo, H. M. Cuppen, C. Romanzin +2

Water is the main component of interstellar ice mantles, is abundant in the solar system and is a crucial ingredient for life. The formation of this molecule in the interstellar me…

astro-ph.SR2010★ 33 cited

H2 reformation in post-shock regions

H. M. Cuppen, L. E. Kristensen, E. Gavardi

H2 formation is an important process in post-shock regions, since H2 is an active participant in the cooling and shielding of the environment. The onset of H2 formation therefore h…