Molecule formation on surfaces of astrophysical interest at low temperatures

Details Molecule formation on surfaces of astrophysical interest at low temperatures Molecule formation on surfaces of astrophysical interest at low temperatures

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msl..confe..49p&link_type=abstract

"Molecules in Space and Laboratory, meeting held in Paris, France, May 14-18, 2007. Editors: J.L. Lemaire, F. Combes. ISBN: 9782

Astronomy and Astrophysics

Astrophysics

Laboratory

Scientific paper

The formation of molecules on the surface of interstellar dust grains plays a fundamental role to enrich the chemical complexity of species observed in space that cannot form efficiently in the gas phase. We give a short presentation with a slight historical perspective of laboratory investigations about reactions catalyzed on interstellar grain nalogues, focusing attention on molecular hydrogen and carbon dioxide.

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