Distributions of metallicity and gas-to-dust ratio in the Magellanic system Kengo Tachihara, Hiroaki Yamamoto, Kisetsu Tsuge, Hidetoshi Sano, and Yasuo.

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Distributions of metallicity and gas-to-dust ratio in the Magellanic system Kengo Tachihara, Hiroaki Yamamoto, Kisetsu Tsuge, Hidetoshi Sano, and Yasuo Fukui (Nagoya University) LMC Magellanic stream Magellanic bridge SMC Slope of the WHI-𝜏353 correlation is a good indicator of metallicity The ISM is the Magellanic system is a mixed gas from LMC and SMC by the dynamical interaction, which triggered active star formation Galactic latitude Galactic longitude SMC Magellanic bridge WHI (K km/s) L-component LMC D-component Magellanic stream Planck dust opacity 𝜏353

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