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And, in particular, when does dust mass growth become dominant as a source of dust mass?
In other words, the dust mass growth becomes less significant.
This accretion process is called "dust mass growth".
Thus, dust produced by dust mass growth becomes the dominant contribution to the dust mass of a galaxy if Z > Zcr in the galaxy.
In Subsection 2.2, we adopted the balance between the dust mass growth by accretion and the dust mass loss by shock destruction (Eq. (6)) as a constraint.
Fig. 3. Left: Percentage of dust mass carried by Fe as a function ol the gas-to-dust mass ratio Rg/d (from Frisch and Slavin, 2003).
Fig. 5. Time evolution of the total dust mass with (solid line) and without (other lines) metallicity dependence for the dust mass growth timescale.
After dust mass growth has taken place, the effect of dust destruction by SN shocks approaches that of dust mass growth.
The next question is what controls the point where the dust mass growth in the ISM dominates the total dust mass production in galaxies.
However, the dust mass in galaxies does not depend on md after accretion growth becomes active.
Hence, δ before the dust mass growth becomes dominant is determined by δstar.
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