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Fig. 23

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Comparison of ice abundances relative to that of H2O for the high-mass sources IRAS 18089 and IRAS 23385 (top) versus the low-mass protostars NGC 1333 IRAS2A and B1-c (bottom). White arrows indicate upper limits. The IRAS2A and IRAS 23385 results are taken from Rocha et al. (2024) and B1-c from Chen et al. (2024).
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