Investigations of Formation of Molecular Hydrogen on Dust Grain Analogues

Details Investigations of Formation of Molecular Hydrogen on Dust Grain Analogues Investigations of Formation of Molecular Hydrogen on Dust Grain Analogues

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nla..work..224v&link_type=abstract

NASA Laboratory Astrophysics Workshop, held May 1-3 2002 at NASA Ames Research Center, Moffett Field, CA 94035-1000. Publisher:

Astronomy and Astrophysics

Astrophysics

Scientific paper

In the last four years we have been working to investigate the formation of molecular hydrogen on surfaces of materials of astrophysical interest, such as silicates, carbonaceous particles and ices, and in conditions approximating the ones present in a variety of astrophysical environments. Our experimental studies - the first of their kind and complemented with computer simulations and theoretical analyses - have given not only hydrogen recombination rates under different ISM conditions, hut they have also offered new insights into this fundamental astrophysical problem. Here we summarize our experimental methods and most significant results.

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