a) Core-corrected bolometric X-ray luminosity versus dynamical mass for the 63 clusters with the best power-law fits for the 63 and 57 (n_gal ≥ 45) clusters as black solid and dashed lines, respectively. b) Core-corrected X-ray bolometric luminosity versus dynamical mass for the 57 (n_gal ≥ 45) clusters with the best power-law fits for the NCC, CC, disturbed, and undisturbed clusters as red dashed, blue dashed, black dot-dot-dot-dashed, and black dotted lines, respectively.