Abstract
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.
Original language | English (US) |
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Pages (from-to) | L131-L134 |
Journal | Astrophysical Journal |
Volume | 483 |
Issue number | 2 PART II |
DOIs | |
State | Published - 1997 |
Keywords
- Dust, extinction
- ISM: abundances
- ISM: molecules
- Molecular processes
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science