363 citations · 3.3k across the 50 of their papers we have counts for
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Reaction Networks For Interstellar Chemical Modelling: Improvements and Challenges
V. Wakelam, I. W. M. Smith, E. Herbst +10
We survey the current situation regarding chemical modelling of the synthesis of molecules in the interstellar medium. The present state of knowledge concerning the rate coefficien…
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…
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…
Molecular dynamics simulations of the ice temperature dependence of water ice photodesorption
C. Arasa, S. Andersson, H. M. Cuppen +2
The ultraviolet (UV) photodissociation of amorphous water ice at different ice temperatures is investigated using molecular dynamics (MD) simulations and analytical potentials. Pre…
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…
Methanol maps of low-mass protostellar systems: the Serpens Molecular Core
L. E. Kristensen, E. F. van Dishoeck, T. A. van Kempen +4
Observations of Serpens have been performed at the JCMT using Harp-B. Maps over a 4.5'x5.4' region were made in a frequency window around 338 GHz, covering the 7-6 transitions of m…