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664 ReferencesMarder, L.(1969).Gravitational waves in general relativity.XI.Cylindrical-sphericalwaves.Proc. Roy. Soc. Lond. A 313, 83.See §22.3.Marek, J.(1968).Some solutions of Einstein’s equations in general relativity.Proc.Camb. Phil. Soc. 64, 167.See §20.6.Mariot, L.(1954).Le champ électromagnétique singulier. C. R. Acad. Sci. (Paris) 238,2055.See §7.6.Marklund, M.(1997).Invariant construction of solutions to Einstein’s field equations –LRS perfect fluids I.CQG 14, 1267.See §§9.4, 13.4, 14.3.Marklund, M.and Bradley, M (1999).Invariant construction of solutions to Einstein’sfield equations – LRS perfect fluids II.CQG 16, 1577.See §§9.4, 16.2.Marklund, M.and Perjés, Z.(1997).Stationary rotating matter in general relativity.JMP 38, 5880.See §19.6.Mars, M.(1995).New non-separable diagonal cosmologies.CQG 12, 2831.See §23.3.Mars, M.(1999).3+1 description of silent universes: a uniqueness result for the Petrovtype I vacuum case.CQG 16, 3245.See §6.2.Mars, M. and Senovilla, J.M.M. (1993a). Axial symmetry and conformal Killingvectors.CQG 10, 1633.See §§19.1, 35.4.Mars, M. and Senovilla, J.M.M. (1993b). Geometry of general hypersurfaces inspacetime – junction conditions.CQG 10, 1865.See §3.8.Mars, M. and Senovilla, J.M.M. (1994). Stationary and axisymmetric perfect fluidsolutions with conformal motion.CQG 11, 3049.See §§21.2, 33.3, 35.4.Mars, M. and Senovilla, J.M.M. (1996). Study of a family of stationary and axiallysymmetric differentially rotating perfect fluids.PRD 54, 6166.See §21.2.Mars, M.and Senovilla, J.M.M. (1997). Non-diagonal G 2 separable perfect-fluidspacetimes.CQG 14, 205.See §23.3.Mars, M. and Senovilla, J.M.M. (1998). On the construction of global models describingrotating bodies; uniqueness of the exterior gravitational field.Mod. Phys. Lett. A13, 1509.See §21.2.Mars, M.and Wolf, T.(1997).G 2 perfect-fluid cosmologies with a proper conformalKilling vector.CQG 14, 2303.See §§23.3, 33.3, 35.4.Martín, J. and Senovilla, J.M.M. (1986). Petrov type D perfect-fluid solutions ingeneralized Kerr–Schild form.JMP 27, 2209.See §§32.5, 33.3.Martín P., F. and Senovilla, J.M.M. (1988). Petrov types D and II perfect-fluidsolutions in generalized Kerr–Schild form.JMP 29, 937.See §32.5.Martinez, E.and Sanz, J.L.(1985).Space-times with intrinsic symmetries on thethree-spaces t = constant.JMP 26, 785.See §36.4.Martins, M.A.P. (1996). The sources of the A and B degenerate static vacuum fields.GRG 28, 1309.See §20.2.Mason, D.P. and Pooe, C.A. (1987). Rotating rigid motion in general relativity. JMP28, 2705.See §6.2.Masuda, T., Sasa, N. and Fukuyama, T. (1998). Neugebauer–Kramer solutions of theErnst equation in Hirota’s direct method.J. Phys. A 31, 5717.See §34.7.Matos, T.and Plebański, J.F. (1994). Axisymmetric stationary solutions as harmonicmaps.GRG 26, 477.See §34.1.Matsumoto, M.(1950).Riemann spaces of class two and their algebraic characterization.JMP(Japan) 2, 67.See §37.5.Matte, A.(1953).Sur de nouvelles solutions oscillatoires des équations de la gravitation.Can. J. Math. 5, 1.See §§3.5, 4.2.May, T.L. (1975). Uniform model universe containing interacting blackbody radiationand matter with internal energy.Astrophys. J. 199, 322.See §14.2.Mazur, P.O. (1983). A relationship between the electrovacuum Ernst equations andnonlinear σ-model.Acta Phys. Polon. B 14, 219.See §34.8.McIntosh, C.(1978a).Self-similar cosmologies with equation of state p = µ. Phys. Lett.A 69, 1.See §§11.4, 23.1.

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