KRATOS: A large suite of N-body simulations to interpret the stellar kinematics of LMC-like discs

Open Access

Fig. 9.

Same as Fig. 8 but for the G_LMC off-centre bar. The evolution of the G_LMC bar off-centredness is given by the distance between the centre of mass of G_LMC and the G_LMC bar centre obtained using a KDE of 3.0 kpc bandwidth as explained in Sect. 2.3.

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