This work investigates the production of molecular hydrogen isotopologues (H2, HD, and D2) during low energy electron irradiation of layered and isotopically labelled thin films of amorphous solid water (ASW) in ultrahigh vacuum. Experimentally, the production of these molecules with both irradiation time and incident electron energy in the range 400 to 500 eV is reported as a function of the depth of a buried D2O layer in an H2O film. H2 is produced consistently in all measurements, reflecting the H2O component of the film, though it does exhibit a modest reduction in intensity at the time corresponding to product escape from the buried D2O layer. In contrast, HD and D2 production exhibit peaks at times corresponding to product escape from...
The results of experiments on the formation of molecular hydrogen on low density and high density am...
Chemical processes on the surface of icy grains play an important role in the chemical evolution in ...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
This work investigates the production of molecular hydrogen isotopologues (H2, HD, and D2) during lo...
To understand elementary processes leading to H{sub 2} formation, and the hydrogenation and deuterat...
Electron-promoted desorption (EPD) from compact amorphous solid water (c-ASW) has been studied. Low-...
In this paper, we report on the formation of molecular hydrogen on different types of amorphous wate...
A common misconception is that outer space is too harsh of an environment to support the production ...
A hydrogen molecule that is formed on an interstellar grain might retain some of the 4.48 eV of ener...
The study of the formation of molecular hydrogen on low temperature surfaces is of interest both bec...
First General Meeting in Prague, May 25 - 29, 2015; http://prague2015astrohistory.vscht.cz/Cold plas...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
Water and some organic molecules were found to be deuterium enriched toward various astronomical tar...
International audienceContext. The synthesis of water is one necessary step in the origin and develo...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
The results of experiments on the formation of molecular hydrogen on low density and high density am...
Chemical processes on the surface of icy grains play an important role in the chemical evolution in ...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
This work investigates the production of molecular hydrogen isotopologues (H2, HD, and D2) during lo...
To understand elementary processes leading to H{sub 2} formation, and the hydrogenation and deuterat...
Electron-promoted desorption (EPD) from compact amorphous solid water (c-ASW) has been studied. Low-...
In this paper, we report on the formation of molecular hydrogen on different types of amorphous wate...
A common misconception is that outer space is too harsh of an environment to support the production ...
A hydrogen molecule that is formed on an interstellar grain might retain some of the 4.48 eV of ener...
The study of the formation of molecular hydrogen on low temperature surfaces is of interest both bec...
First General Meeting in Prague, May 25 - 29, 2015; http://prague2015astrohistory.vscht.cz/Cold plas...
International audienceThe gas-surface interaction of molecular hydrogen D 2 with a thin film of poro...
Water and some organic molecules were found to be deuterium enriched toward various astronomical tar...
International audienceContext. The synthesis of water is one necessary step in the origin and develo...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
The results of experiments on the formation of molecular hydrogen on low density and high density am...
Chemical processes on the surface of icy grains play an important role in the chemical evolution in ...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...