Fig. 8
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Density contrast maps of the AURIGA 2 simulation for three distinct age intervals: stellar particles younger than 1 Gyr (left column), those aged between 1 and 2 Gyr (middle column), and those between 2 and 3 Gyr (right column). Open circles indicate the spiral arm tracks inferred from Fig. 3. Cross in the bottom-right corner indicates the scale of ±5 kpc.
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