197 citations · 1.4k across the 22 of their papers we have counts for
22 papers
Efficient Interstellar Grain Growth from High Sticking Coefficients on Amorphous Carbon Dust
Clarke J. Esmerian, Duncan Bossion, Francois Dulieu +8
Cosmic dust is the solid phase of the interstellar medium (ISM), classically assumed to be composed of carbonaceous and silicate grains with size distributions spanning …
Astrochemical models of interstellar ices: History matters
A. Clément, A. Taillard, V. Wakelam +6
Ice is ubiquitous in the interstellar medium. We model the formation of the main constituents of interstellar ices, including H2O, CO2 , CO, and CH3 OH. We strive to understand wha…
Ammonia snow-lines and ammonium salts desorption
F. Kruczkiewicz, J. Vitorino, E. Congiu +2
Context. The nitrogen reservoir in planetary systems is a long standing problem. Part of the N-bearing molecules is probably incorporated into the ice bulk during the cold phases o…
Thermal desorption of formamide and methylamine from graphite and amorphous water ice surfaces
Henda Chaabouni, Stephan Diana, Thanh Nguyen +1
Formamide (NH2CHO) and methylamine (CH3NH2) are known to be the most abundant amine-containing molecules in many astrophysical environments. The presence of these molecules in the…
H formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
Valentine Wakelam, Emeric Bron, Stephanie Cazaux +12
Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form and survive photo-dissociation in tenuous environments. Its formation involves catalyt…
Deuteration of ammonia with D atoms on oxidized partly ASW covered graphite surface
Henda Chaabouni, Marco Minissale, Saoud Baouche +1
The deuteration of ammonia by D atoms has been investigated experimentally in the sub-monolayer regime on realistic analogues of interstellar dust grain surfaces. About 0.8 monolay…