Upper panels: distribution of bulge stars with frequency (Ω−Ω_B) /κ at different times throughout the secular evolution in model RHG097. Lower panels: net change in the angular momentum of the selected stars with respect to the previous time. The vertical dotted lines indicate the most important resonances (from left to right): −1:1, 4:1, 3:1, 5:2, and 2:1. As time progresses, more stars are trapped by the ILR of the bar in the stellar disk. However, most of the angular momentum transfer occurs through the 5:2 resonance.