H2 formation on interstellar grains in different physical regimes

O. Biham*, I. Furman, N. Katz, V. Pirronello, G. Vidali

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

44 Scopus citations

Abstract

An analysis of the kinetics of H2 formation on interstellar dust grains is presented using rate equations. It is shown that semi-empirical expressions that have appeared in the literature represent two different physical regimes. In particular, it is shown that the expression given by Hollenbach, Werner & Salpeter applies when high flux, or high mobility, of H atoms on the surface of a grain makes it very unlikely that H atoms evaporate before they meet each other and recombine. The expression of Pirronello et al. - deduced on the basis of accurate measurements of a realistic dust analogue - applies to the opposite regime (low coverage and low mobility). The implications of this analysis for the understanding of the processes dominating in the interstellar medium are discussed.

Original languageAmerican English
Pages (from-to)869-872
Number of pages4
JournalMonthly Notices of the Royal Astronomical Society
Volume296
Issue number4
DOIs
StatePublished - 1 Jun 1998

Keywords

  • Atomic processes
  • ISM: abundances
  • ISM: atoms
  • ISM: molecules
  • Molecular processes

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