Fig. 14
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Measured intensities of H I-1 and CN band peak relative to Mg I-2 in spectra of tested meteorites. H line intensity in meteorites BIL, LUN, and EAG may be affected by a contaminant source of H. Regions characteristic for meteorite spectra with no confirmed H or CN emission are marked in color. The meteorite group color coding is the same as in other figures in this work.
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