In Auriga simulations, boxy/peanut bulges form 1.1-1.6 Gyr after bar formation, always after a buckling event, and appear in 45% of barred galaxies at z=0, dropping to zero by z~1.
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Formation and evolution of boxy/peanut bulges in the Auriga cosmological simulations
In Auriga simulations, boxy/peanut bulges form 1.1-1.6 Gyr after bar formation, always after a buckling event, and appear in 45% of barred galaxies at z=0, dropping to zero by z~1.