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Density-dependent relations among saturation properties of symmetric nuclearmatter and hyperonic matter, properties of hadron-(strange) quark hybrid starsare discussed by applying the conserving nonlinear $\sigma$-$\omega$-$\rho$hadronic mean-field theory. Nonlinear interactions that will be renormalized aseffective coupling constants, effective masses and sources of equations ofmotion are constructed self-consistently by maintaining thermodynamicconsistency to the mean-field approximation. The coupling constants expectedfrom the hadronic mean-field model and SU(6) quark model for the vectorcoupling constants are compared; the coupling constants exhibit differentdensity-dependent results for effective masses and binding energies ofhyperons, properties of hadron and hadron-quark stars. The nonlinear$\sigma$-$\omega$-$\rho$ hadronic mean-field approximation with or withoutvacuum fluctuation corrections and strange quark matter defined by MIT-bagmodel are employed to examine properties of hadron-(strange) quark hybridstars. We have found that hadron-(strange) quark hybrid stars become morestable in high density compared to pure hadronic and strange quark stars.

Hardon-quark hybrid stars constructed by the nonlinear $\sigma$-$\omega$-$\rho$ mean-field model and MIT-bag model