Fig. 10.

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Evolution of disk gas at different redshifts. For each snapshot at a given redshift z, gas particles that are cold and in the disk are tracked forward until an outcome is identified: the particle is heated within the disk, the particle is launched in an outflow but is still cold, the particle is launched in an outflow and is heated above T0, or the particle is converted into stars. If none of the previous outcomes is found earlier than z = 0.3, it means that the particle remains cold in the disk. Left: total mass of the gas in each outcome. Right: fraction of the gas mass in each outcome, with respect to the initial cold disk gas at the redshift z at which the forward tracking is started.
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