The chiral phase transition of a hot and dense system of quarks is stu
died within a modified SU(3) NJL Lagrangian that implements the QCD sc
ale anomaly. The u- and s-quark condensates can or can not feel the sa
me chiral restoration depending on the considered region of the three-
dimensional space (T-c, mu(uc), mu(sc)) The temperature behaviour of t
he pressure and the energy and entropy densities of the u- and s-quark
system is investigated. At high temperature, the nonvanishing bare s-
quark mass only modifies slightly the usual behaviour associated with
an ideal quark gas.