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Three types of magnetic phase diagrams as a function of composition or pressure, f ( z , p ), are identified among Ce systems: I) with the ordering temperature T ord →0 monotonously, followed by a narrow region where non-Fermi-liquid (NFL) behavior is observed; II) with T ord vanishing at finite temperature, but followed by an extended NFL region, and III) where T ord remains nearly constant. Among the analyzed systems intrinsic differences are found in the evolution of their respective properties, namely: in group-I an increase of the density of excitations is observed below T ord . In group-II the evanescense of T ord ( z , p ) coincides with the extrapolation to zero of the magnetic free energy (Δ G →0), and the existence of a reference function implying that T K ≠ f ( z , p ), whereas T ord = f ( z , p ). Finally, group-III is also characterized by the evanescense of T ord where Δ G →0, but in this case T ord ≠ f ( z , p ) whereas T K = f ( z , p ). The characteristics of each group are discussed and compared together with the different C p ( T )/ T dependencies at T ≥ T ord and some related scalings, which allow to recognize a quasi-paramagnetic phase.
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