The adsorption and desorption of CO on and from amorphous H2O ice at astrophysically relevant temperatures has been studied using temperature programmed desorption (TPD) and reflection-absorption infrared spectroscopy (RAIRS). Solid CO is able to diffuse into the porous structure of H2O at temperatures as low as 15 K. When heated, a phase transition between two forms of amorphous H2O ice occurs over the 30-70 K temperature range, causing the partial collapse of pores and the entrapment of CO. Trapped CO is released during crystallization and desorption of the H2O film. This behavior may have a significant impact on both gas-phase and solid-phase chemistry in a variety of interstellar environments
Context. Ice desorption affects the evolution of the gas-phase chemistry during the protos...
We present laboratory data on pure, layered and mixed CO and O-2 ices relevant for understanding the...
The surface processes on interstellar dust grains have an important role in the chemical evolution i...
The adsorption and desorption of CO on and from amorphous H2O ice at astrophysically relevant temper...
The interaction of carbon monoxide (CO) with vapour-deposited water (H2O) ices has been studied usin...
Context. Recent observations of protoplanetary disks suggest that they are depleted in gas-phase CO ...
Molecular ices freeze out on the surface of dust grains within the interstellar medium (ISM). Dust g...
International audienceCarbon monoxide (CO) is the second most abundant molecule in the gas phase of ...
Context. Recent observations of protoplanetary disks suggest that they are depleted in gas-phase CO ...
Context. Ice photodesorption has been the topic of recent studies that aim to interpret the abundanc...
Aims. Solid O2 has been proposed as a possible reservoir for molecular oxygen in dense clouds throug...
Recent results from the Raymond and Beverly Sackler Laboratory for Astrophysics on spectroscopy and ...
Aims.We studied the interaction between CO2 (guest) and H2O (host) molecular ices. Methods....
We present the results of classical trajectory calculations of the adsorption of thermal CO on the s...
Solid O2 has been proposed as a possible reservoir for molecular oxygen in dense clouds through free...
Context. Ice desorption affects the evolution of the gas-phase chemistry during the protos...
We present laboratory data on pure, layered and mixed CO and O-2 ices relevant for understanding the...
The surface processes on interstellar dust grains have an important role in the chemical evolution i...
The adsorption and desorption of CO on and from amorphous H2O ice at astrophysically relevant temper...
The interaction of carbon monoxide (CO) with vapour-deposited water (H2O) ices has been studied usin...
Context. Recent observations of protoplanetary disks suggest that they are depleted in gas-phase CO ...
Molecular ices freeze out on the surface of dust grains within the interstellar medium (ISM). Dust g...
International audienceCarbon monoxide (CO) is the second most abundant molecule in the gas phase of ...
Context. Recent observations of protoplanetary disks suggest that they are depleted in gas-phase CO ...
Context. Ice photodesorption has been the topic of recent studies that aim to interpret the abundanc...
Aims. Solid O2 has been proposed as a possible reservoir for molecular oxygen in dense clouds throug...
Recent results from the Raymond and Beverly Sackler Laboratory for Astrophysics on spectroscopy and ...
Aims.We studied the interaction between CO2 (guest) and H2O (host) molecular ices. Methods....
We present the results of classical trajectory calculations of the adsorption of thermal CO on the s...
Solid O2 has been proposed as a possible reservoir for molecular oxygen in dense clouds through free...
Context. Ice desorption affects the evolution of the gas-phase chemistry during the protos...
We present laboratory data on pure, layered and mixed CO and O-2 ices relevant for understanding the...
The surface processes on interstellar dust grains have an important role in the chemical evolution i...