Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...147...54d&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 147, no. 1, June 1985, p. 54-60. Research supported by the Centre National d'E
Astronomy and Astrophysics
Astrophysics
Chemical Evolution, Graphite, High Energy Interactions, Interstellar Matter, Molecular Interactions, Synthesis (Chemistry), Cosmic Dust, Cosmic Plasma, Molecular Beams, Vacuum Chambers
Scientific paper
The objective of this paper is to show a possibility of forming interstellar molecules detected in the interstellar space by bombarding a carbon target or graphite grains with high energy neutrals. The authors have bombarded pure graphite in the ultra-vacuum with high energy molecular beams (from 2 to 10 keV) obtained by charge exchange from ion beams of hydrogen, oxygen, or nitrogen. They have observed many organic compounds: binary compounds like hydrogen carbides, ternary compounds containing carbon, nitrogen, oxygen or hydrogen, and finally, quaternary compounds. They also have obtained cyanopolyynes and organic molecules which had previously been observed in the interstellar space. So far, they have identified thirty-two compounds corresponding to molecules observed in the interstellar space and about forty containing only carbon, hydrogen, nitrogen and oxygen.
Devienne F. M.
Teisseire Maguelonne
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