Locations of the blue and red edges for fundamental mode pulsation. The left panel is for models of the solar metallicity with various initial rotation rates, while the right panel is for models of an initial rotation of ω_ini = 0.5 with various metal abundances. The thinner lines show the locations of blue edges obtained with the frozen convection assumption, while the thicker lines show blue and red edges obtained by taking into account the perturbation of convection flux. The left panel also shows the positions of some Galactic Cepheids whose parameters are taken from Turner & Burke (2002), Turner et al. (2012, 2013), and Turner (2013).