Molecular and mass spectroscopic analysis of isotopically labeled organic residues.

Details Molecular and mass spectroscopic analysis of isotopically labeled organic residues. Molecular and mass spectroscopic analysis of isotopically labeled organic residues.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.257m&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 257 - 260

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Organic Molecules: Evolution, Organic Molecules: Interstellar Grains

Scientific paper

Experimental studies aimed at understanding the evolution of complex organic molecules on interstellar grains have been performed. The photolysis of frozen gas mixtures of various composition containing H2O; CO; NH3 and CH4 was studied. These ultraviolet photolysed ices were warmed up in order to produce refractory organic molecules like the ones formed in molecular clouds when the icy mantles are being irradiated and warmed up either by a nearby stellar source or impulsive heating. The laboratory studies give us among other results, estimates of the efficiency of production of such organic material under interstellar conditions.

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