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The growth and the evolution of the bar instability in stellar-gaseous disks embedded in a dark matter halo evolving in a cosmological framework is explored. We point out the impact of different gas fractions on the bar formation, inside disks of different disk-to-halo mass ratio.doi:10.1017/s1743921306010295 fatcat:42yena5yqnfblfl32a2z7f3xr4