To understand elementary processes leading to H{sub 2} formation, and the hydrogenation and deuteration reactions of adsorbed species on dust grains in dense clouds, we experimentally investigated the diffusion of atomic hydrogen and deuterium on amorphous solid water (ASW) at temperatures of 8-15 K. The present study extended our previous study for selective detections of H and D atoms, and of H{sub 2} (J = 0 and 1) and D{sub 2} (J = 0 and 1) molecules adsorbed on ASW using both photo-stimulated desorption and resonance-enhanced multiphoton ionization, to investigate potential sites on ASW for diffusion, recombination dynamics, and the diffusion mechanism of H and D atoms. Our results demonstrate that the ASW surface contains various poten...
In this paper, we report on the formation of molecular hydrogen on different types of amorphous wate...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H-2, is generally thought to form by recombination of H ato...
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...
The study of the formation of molecular hydrogen on low temperature surfaces is of interest both bec...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
A hydrogen molecule that is formed on an interstellar grain might retain some of the 4.48 eV of ener...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
In this paper, we report on the formation of molecular hydrogen on different types of amorphous wate...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H-2, is generally thought to form by recombination of H ato...
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...
The study of the formation of molecular hydrogen on low temperature surfaces is of interest both bec...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
Aims. The mobility of H atoms on the surface of interstellar dust grains at low temperature is still...
The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are imp...
A hydrogen molecule that is formed on an interstellar grain might retain some of the 4.48 eV of ener...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
In this paper, we report on the formation of molecular hydrogen on different types of amorphous wate...
The most abundant interstellar molecule, H2, is generally thought to form by recombination of H atom...
The most abundant interstellar molecule, H-2, is generally thought to form by recombination of H ato...