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Fig. 5
Surface brightness of the remnant in our simulations, assuming a stellar mass-to-light ratio in the V-band of γ∗ = 2.1 for the M1 model on the upper panel and γ∗ = 2.4 for the M2 model in the lower panel. The surface brightness in both cases is μ0 ≈ 24.6 mag/arcsec2. Compare this plot to Figure 4 of Majewski et al. (2003).
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