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A full (3+1)-dimensional calculation using the Lagrangian hydrodynamics isproposed for relativistic nuclear collisions. The calculation enables us toevaluate anisotropic flow of hadronic matter which appears in non-centraland/or asymmetrical relativistic nuclear collisions. Applying hydrodynamicalcalculations to the deformed uranium collisions at AGS energy region, wediscuss the nature of space-time structure and particle distributions indetail.Comment: 24 pages, 25 eps figures, LaTeX 2 epsilo

(3+1)-dimensional relativistic hydrodynamical expansion of hot and dense matter in ultra-relativistic nuclear collision