In a NIHAO-UHD Milky Way analogue, Splash-like stars were already born on dynamically hot orbits; the last major merger did not significantly heat them.
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The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- II. Were Splash stars heated or already born hot?
In a NIHAO-UHD Milky Way analogue, Splash-like stars were already born on dynamically hot orbits; the last major merger did not significantly heat them.