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Fig. 14.
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Upper panel: SFR evolution of gas-poor major merger analogous to VCC 479. Middle panel: Stellar particle map overlaid with HI gas contours at 0.5, 5, and 50 M⊙ pc−2 for the gas-poor merger. The stellar map is expressed in units of solar masses per square parsec. Bottom panel: Stellar map of the gas-rich merger.
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