activity
20092024
most citedExperimental evidence for water formation via ozone hydrogenation on dust grains at 10 K

108 citations · 348 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024★ 4 cited

Photocleavage of aliphatic C--C bonds in the interstellar medium

Guillermo Tajuelo-Castilla, Jesús I. Mendieta-Moreno, Mario Accolla +6

Ultraviolet (UV) processing in the insterstellar medium (ISM) induces the dehydrogenation of hydrocarbons. Aliphatics, including alkanes, are present in different interstellar envi…

astro-ph.IM2020★ 7 cited

INFRA-ICE: an ultra-high vacuum experimental station for laboratory astrochemistry

Gonzalo Santoro, Jesús. M. Sobrado, Guillermo Tajuelo-Castilla +7

Laboratory astrochemistry aims at simulating in the laboratory some of the chemical and physical processes that operate in different regions of the Universe. Amongst the diverse as…

astro-ph.GA2020★ 18 cited

Silicon and hydrogen chemistry under laboratory conditions mimicking the atmosphere of evolved stars

Mario Accolla, Gonzalo Santoro, Pablo Merino +10

Silicon is present in interstellar dust grains, meteorites and asteroids, and to date thirteen silicon-bearing molecules have been detected in the gas-phase towards late-type stars…

astro-ph.GA2020★ 45 cited

The chemistry of cosmic dust analogues from C, C, and CH in C-rich circumstellar envelopes

Gonzalo Santoro, Lidia Martínez, Koen Lauwaet +13

Interstellar carbonaceous dust is mainly formed in the innermost regions of circumstellar envelopes around carbon-rich asymptotic giant branch (AGB) stars. In these highly chemical…

cond-mat.mtrl-sci2014★ 62 cited

Quantum tunneling of oxygen atoms on very cold surfaces

M. Minissale, E. Congiu, S. Baouche +7

Any evolving system can change of state via thermal mechanisms (hopping a barrier) or via quantum tunneling. Most of the time, efficient classical mechanisms dominate at high tempe…

astro-ph.GA2010★ 60 cited

Changes in the morphology of interstellar ice analogues after hydrogen atom exposure

Mario Accolla, Emanuele Congiu, François Dulieu +6

The morphology of water ice in the interstellar medium is still an open question. Although accretion of gaseous water could not be the only possible origin of the observed icy mant…

physics.chem-ph2010★ 44 cited

Gas temperature dependent sticking of hydrogen on cold amorphous water ice surfaces of interstellar interest

E. Matar, H. Bergeron, F. Dulieu +3

Using the King & Wells method, we present experimental data on the dependence of the sticking of molecular hydrogen and deuterium on the beam temperature onto non- porous amorphous…

astro-ph.GA2009★ 108 cited

Experimental evidence for water formation via ozone hydrogenation on dust grains at 10 K

H. Mokrane, H. Chaabouni, M. Accolla +4

The formation of water molecules from the reaction between ozone (O3) and D-atoms is studied experimentally for the first time. Ozone is deposited on non-porous amorphous solid wat…