Interstellar absorptions at 3.2 microns and 3.3 microns

Details Interstellar absorptions at 3.2 microns and 3.3 microns Interstellar absorptions at 3.2 microns and 3.3 microns

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8318625a&link_type=abstract

In its Organo-Siliceous Biomolecules and the Infrared Spectrum of the Trapezium Nebula and Interstellar Absorptions at 3.2 Micro

Astronomy and Astrophysics

Astronomy

Amino Acids, Exobiology, Infrared Absorption, Infrared Astronomy, Interstellar Matter, Absorption Spectra, Bacteria, Interstellar Chemistry

Scientific paper

In a recent attempt to interpret the IR spectrum of the source GC-IRS 7 on the basis of a bacterial strain model (Hoyle et al., 1982), two absorption features at 3.2 and 3.3 microns remained unexplained. It is suggested that NH3(+) vibrations due to free amino acids in bacterial grains may provide a self-consistent explanation of the unidentified absorptions in the IR.

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