The IR spectrum of laboratory synthesized polymeric residues

Details The IR spectrum of laboratory synthesized polymeric residues The IR spectrum of laboratory synthesized polymeric residues

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...133...77s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 133, no. 1, April 1984, p. 77-79.

Astronomy and Astrophysics

Astrophysics

24

Cosmochemistry, Hydrocarbons, Infrared Spectra, Interstellar Matter, Polymerization, Synthesis (Chemistry), Environmental Laboratories, Granular Materials, Interstellar Radiation, Potassium Bromides, Proton Energy, Residues, Space Environment Simulation

Scientific paper

The IR spectra of solid residues obtained by bombarding hydrocarbons frozen on KBr matrices with fast protons are presented. A common dominant IR feature near 3.4 μm resembles that observed in some astrophysical sources. These results and others obtained by bombarding C-rich mixtures suggest that the 3.4 μm feature, typical of -CH2 and -CH3 groups, is produced independently of the original hydrocarbon and of the physical conditions during the condensation.

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