A 1:4 major merger simulation with a chemical model reproduces the chemodynamical properties of M31's Giant Stellar Stream and NE/W shelves, supporting a recent major merger.
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The survey of planetary nebulae in Andromeda (M31) VII. Predictions of a major merger simulation model compared with chemodynamical data of the disc and inner halo substructures
A 1:4 major merger simulation with a chemical model reproduces the chemodynamical properties of M31's Giant Stellar Stream and NE/W shelves, supporting a recent major merger.