The NewHorizon simulation – to bar or not to bar

The NewHorizon simulation – to bar or not to bar

We use the NEWHORIZON simulation to study the redshift evolution of bar properties and fractions within galaxies in the stellar masses range M⋆ = 107.25–1011.4M⊙ over the redshift range of z = 0.25–1.3. We select disc galaxies using stellar kinematics as a proxy for galaxy morphology. We employ two...

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Bibliographic Details
Main Authors:	Reddish, J, Kraljic, K, Petersen, MS, Tep, K, Dubois, Y, Pichon, C, Peirani, S, Bournaud, F, Choi, H, Devriendt, J, Jackson, R, Martin, G, Park, MJ, Volonteri, M, Yi, SK
Format:	Journal article
Language:	English
Published:	Oxford University Press 2022

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