Notes. M_h is the halo mass; a_h is the halo scale length; M_d, R_d, z_d are the initial stellar disk mass, radial scale length and vertical scale height respectively; M_gas, R_gas, z_gas are the initial stellar disk mass, radial scale length and vertical scale hight respectively; r_b is the bar size; ε_b is the bar potential amplitude; h is the bar growth timescale in models with a rigid bar potential. Models marked by minus include no converging flow criterion in the star-formation prescription. First section of the table shows the model with no bar imposed in the disk (axisymmetric potential); the second section presents models with a rigid potential of bar; and the last section shows the parameters of the self-consistent simulations that have live halos and an initial stellar disk. For simulations with a rigid potential, we adopted an isothermal dark matter (iso) distribution and exponential (exp) stellar disk; for self-consistent simulations we used Plummer (plum) sphere for dark matter halo and Miyamoto-Nagai (M-N) initial stellar disk.