International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of porous amorphous solid water ͑ASW͒ grown at 10 K by slow vapor deposition has been studied by temperature-programed-desorption ͑TPD͒ experiments. Molecular hydrogen diffuses rapidly into the porous network of the ice. The D 2 desorption occurring between 10 and 30 K is considered here as a good probe of the effective surface of ASW interacting with the gas. The desorption kinetics have been systematically measured at various coverages. A careful analysis based on the Arrhenius plot method has provided the D 2 binding energies as a function of the coverage. Asymmetric and broad distributions of binding energies were found, with a maximum populatio...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
The molecular hydrogen, a major component of the interstellar medium (ISM) isformed on dust grains t...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
International audienceAims: The mobility of H atoms on the surface of interstellar dust grains at lo...
International audienceAims: The mobility of H atoms on the surface of interstellar dust grains at lo...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
The molecular hydrogen, a major component of the interstellar medium (ISM) isformed on dust grains t...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
International audienceThe desorption kinetics of D 2 from amorphous solid water (ASW) films have bee...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
International audienceAims: The mobility of H atoms on the surface of interstellar dust grains at lo...
International audienceAims: The mobility of H atoms on the surface of interstellar dust grains at lo...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
The molecular hydrogen, a major component of the interstellar medium (ISM) isformed on dust grains t...