Infra-red absorption lines by molecules in grain mantles

Details Infra-red absorption lines by molecules in grain mantles Infra-red absorption lines by molecules in grain mantles

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86l...3h&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 1-2, June 1980, p. L3-L6. Research supported by the Alexander von Humboldt-Stiftung.

Astronomy and Astrophysics

Astronomy

45

Absorption Spectra, Astronomical Models, Infrared Absorption, Molecular Absorption, Radio Sources (Astronomy), Cores, Galactic Nuclei, Line Spectra, Microwave Spectra, Radiant Flux Density, Radio Galaxies

Scientific paper

The laboratory spectrum of a solid mixture of H2O, CO, CH3OH, and NH3 at a temperature of 10 K reproduces the shape and peak positions of interstellar features. It is shown that the broad absorption features evident in the MIR spectra of some astronomical objects associated with interstellar dust can be explained by absorptions of molecules in grain mantles.

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