Fig. 8
History of the extended disk in Malin 1 according to our best-fit model. Left: evolution at specific radii (28, 55, and 110 kpc). Right: evolution of integrated quantities (over the full disk modeled, or within about 110 kpc, corresponding to the size of the visible disk). The integrated values are compared to the values of Boissier et al. (2008) for the star-formation rate and Lelli et al. (2010) for the gas (shown by the errorbar in the topmost two right panels).
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