  We compare stellar orbits in an early (NGC 4314) and a late-type barred
galaxy (NGC 1073). We find that these bars are cold in the sense that the
majority of stars can be described as being nearby to periodic orbits. We place
limits of (65km/s)^2 and (50km/s)^2 on the components of the diagonalized
velocity dispersion ellipsoid matrix for stars in the bars of NGC 4314 and NGC
1073 respectively. Both bars end near the inner 4:1 Lindblad (ultraharmonic)
resonance. We conjecture that a large class of bars end near this resonance.
The morphology of the bars depends on the strength of the 4:1 resonance, which
is strong in the early-type barred galaxy and weak in the other. This results
in a flat bar major axis surface brightness profile for the early-type bar and
an exponential profile for the late-type bar.
