Projected edge-on mass-weighted stellar velocity dispersion fields (σ_*) for G11, G70, G31, and G45. Each map has been derived at a specific epoch in which the galaxy is displaying a clear stars-gas counter-rotating configuration. For G11, G70, and G45, the presence of the counter-rotating stellar component cannot be seen in their projected stellar velocity fields but may be suggested by the presence of the double-peak feature exhibited in these maps.