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Fig. 22.
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Estimated CO gas surface densities ΣCO for the gas-poor G9LG_VLZ galaxy (left panels) and the gas-rich G9HG_VLZ galaxy (right panels) at t = 400 Myr. Red are for the isocontours of projected gas density of 10 H cm−3. The gas-rich galaxy produce much more molecular gas mass than the gas-poor galaxy.
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