Comparisons of abundances for SO₂, CH₃OH, and CH₃CN from observations of the seven hot cores detected in this galaxy and the LMC hot core models for the final hot core temperature of 100 K (top) and 200 K (bottom). The black curves show abundances over time for an initial dust temperature of 10 (dotted curve), 15 (dashed curve), 20 (larger dashed curve), and 25 K (the solid curve). The horizontal colored line shows the single abundance value for each hot core and follows the same color code as Fig. 13 (see the text for more details).