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Paper: Barred Galaxies: Dynamical and Chemo-Photometrical Evolution
Volume: 230, Galaxy Disks and Disk Galaxies
Page: 351
Authors: Curir, A.; Mazzei, P.
Abstract: We present smooth particle hydrodynamics (SPH) simulations of barred galaxies with the aim to give insights into the role of the mass and triaxiality of the halo on inhibiting or maintaining the bar instability. We also want to focus the impact of these dynamical parameters on the star formation.
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