Model 1, morphology of the bar-B/P region at t = 5 Gyr. First and third column, from top to bottom: Face-on (Col. 1) and edge-on (Col. 3) absolute stellar densities of all stars (top panel), and stars initially in the cold (second panel), intermediate (third panel), and hot (bottom panel) disks. Second and fourth column, from top to bottom: Fraction of cold- (second panel), intermediate- (third panel), and hot-disk (bottom panel) stars in the B/P bulge, seen face-on (Col. 2) and edge-on (Col. 4). The fraction is defined as the ratio of cold-, intermediate-, or hot-disk stars to the total (i.e., cold+intermediate+hot) disk stars in the B/P bulge. In the edge-on maps, only stars in the bar (|x| ≤ 5.5 kpc and |y| ≤ 3 kpc) have been selected.