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References 617Bach, R.and Weyl, H.(1922).Neue Lösungen der Einsteinschen Gravitationsgleichungen.Math.Z. 13, 134.See §20.2.Baillie, G.and Madsen, M.S.(1985).A tilted Bianchi type-V perfect fluid solution forstiff matter.Astrophys. Space Sci. 115, 413.See §§10.11, 23.1.Bajer, K.and Kowalczyński, J.K. (1985). A class of solutions of the Einstein–Maxwellequations.JMP 26, 1330.See §28.2.Balasin, H.and Nachbagauer, H.(1996).Boosting the Kerr geometry in an arbitrarydirection.CQG 13, 731.See §9.5.Baldwin, O.R. and Jeffery, G.B. (1926). The relativity theory of plane waves. Proc. Roy.Soc. Lond. A 111, 95.See §24.5.Bampi, F.and Cianci, R.(1979).Generalized axisymmetric spacetimes.Commun.Math. Phys. 70, 69.See §§24.3, 24.4, 31.5.Banerjee, A.(1970).Null electromagnetic fields in general relativity admitting timelikeor null Killing vectors.JMP 11, 51.See §18.6.Banerjee, A.K. and Santos, N.O. (1984). Spatially homogeneous cosmological models.GRG 16, 217.See §14.3.Bardeen, J.M. (1970). A variational principle for rotating stars in general relativity.Astrophys. J. 162, 71.See §19.3.Barnes, A.(1972).Static perfect fluids in general relativity.J. Phys. A 5, 374.See §§13.4, 18.6.Barnes, A.(1973a).On Birkhoff’s theorem in general relativity.Commun. Math. Phys.33, 75.See §§8.5, 15.4, 24.1.Barnes, A.(1973b).On shearfree normal flows of a perfect fluid.GRG 4, 105.See §§6.2, 16.2, 15.6, 33.3.Barnes, A.(1973c).Space-times of embedding class one in general relativity.GRG 5,147.See §§37.4, 37.5.Barnes, A.(1977).A class of algebraically general non-null Einstein–Maxwell fields.II.J. Phys. A 10, 755.See §13.3.Barnes, A.(1978).A class of homogeneous Einstein–Maxwell fields.J. Phys. A 11,1303.See §§13.2, 13.3.Barnes, A.(1979).On space-times admitting a three-parameter isometry group withtwo-dimensional null orbits.J. Phys. A 12, 1493.See §§13.1, 24.1.Barnes, A.(1984).Shear-free flow of a perfect fluid, in Classical general relativity, eds.W.B. Bonnor, J.N. Islam and M.A.H. MacCallum, page 15 (Cambridge UniversityPress, Cambridge).See §6.2.Barnes, A.(1998).Symmetries of the Stephani universes.CQG 15, 3061.See §37.4.Barnes, A.(1999).On Stephani’s rotating dust solutions.CQG 16, 919.See §36.3.Barnes, A.(2000).A comment on a paper by Carot et al.CQG 17, 2605. See§19.1.Barnes, A.and Rowlingson, R.R.(1989).Irrotational perfect fluids with a purely electricWeyl tensor.CQG 6, 949.See §6.2.Barnes, A.and Rowlingson, R.R.(1990).Killing vectors in conformally flat perfect fluidspacetimes.CQG 7, 1721.See §37.4.Barrabés, C.(1989).Singular hypersurfaces in general relativity: a unified description.CQG 6, 581.See §3.8.Barrabés, C.and Israel, W.(1991).Thin shells in general relativity and cosmology: thelightlike limit.PRD 43, 1129.See §3.8.Barrow, J.D. (1978).Quiescent cosmology.Nature 272, 211.See §14.4.Barrow, J.D. and Stein-Schabes, J. (1984). Inhomogeneous cosmologies with cosmologicalconstant.Phys. Lett. A 103, 315.See §33.3.Bartrum, P.C. (1967). Null electromagnetic field in the form of spherical radiation. JMP8, 1464.See §28.2.Basey, T.C. (1975).A note on the generation of twisting ‘D’ metrics from non-twisting‘D’ metrics.Z. Naturforsch. 30a, 1200.See §21.1.

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