We report on laboratory measurements of molecular hydrogen formation and recombination on an olivine slab as a function of surface temperature under conditions relevant to those encountered in the interstellar medium. On the basis of our experimental evidence, we recognize that there are two main regimes of H coverage that are of astrophysical importance; for each of them we provide an expression giving the production rate of molecular hydrogen in interstellar clouds.
Vidali, Gianfranco; Pirronello, Valerio; Biham, Ofer; Liu, Chi; and Shen, Lyiong, "Efficiency of Molecular Hydrogen Formation on Silicates" (1997). Physics. Paper 512.
Harvested from Arxiv.org