Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations

Open Access

Table C.1.

Coefficients of the fifth-order polynomial fit for the sputtering rate (i= silicate or carbonaceous grains) $log (Y_{i} / (μ m {yr}^{- 1} {cm}^{3})) = \sum_{n = 0}^{5} a_{n} {(log (T / K))}^{n}$ $\log(Y_i/(\mu \mathrm{m} \, \mathrm{yr^{-1}}\, \mathrm{cm}^3))=\sum\nolimits_{n=0}^5 a_n (\log (T/\mathrm{K}))^n$ of Hu et al. (2019) to the values predicted by Nozawa et al. (2006).

grain type	a₀	a₁	a₂	a₃	a₄	a₅
silicate	-234.791	133.209	-31.3027	3.71345	-0.221824	0.00531746
carbonaceous	-234.334	138.486	-33.9022	4.17705	-0.258281	0.00638828

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