Fig. 13
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Abundances of different molecular species for all the known hot cores in the LMC after scaling to the gas-to-dust mass ratio. The LMC hot cores are ST11 (Shimonishi et al. 2016a), 4A, 6A, 6B and 14A (this work), and N113 Al and N113 B (Sewiło et al. 2022). Black arrows show an upper limit estimation. An error range of 40% is shown on the abundances from the current paper.
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