In Auriga Superstars simulations, old stellar morphological lopsidedness correlates strongly with HI lopsidedness at z=0, with tidal interactions inducing coherent asymmetries in both while smooth accretion primarily affects gas and young stars.
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Coupling between stellar and HI lopsidedness in Milky Way-type galaxies from the Auriga Superstars cosmological simulations
In Auriga Superstars simulations, old stellar morphological lopsidedness correlates strongly with HI lopsidedness at z=0, with tidal interactions inducing coherent asymmetries in both while smooth accretion primarily affects gas and young stars.