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632 ReferencesDemiański, M.and Newman, E.T.(1966).A combined Kerr–NUT solution of theEinstein field equations.Bull. Acad. Polon. Sci. Math. Astron. Phys. 14, 653.See§§20.5, 21.1, 34.1.Denisova, T.E., Khakimov, S.A. and Manko, V.S. (1994). The Gutsunaev–Mankostatic vacuum solution.GRG 26, 119.See §20.2.Denisova, T.E. and Manko, V.S. (1992). Exact solution of the Einstein–Maxwellequations referring to a charged spinning mass.CQG 9, L57.See §34.1.Denisova, T.E., Manko, V.S. and Shorokhov, S.G. (1991). Generalization of theKerr–Newman solution.Sov. Phys. J. 34, 1050.See §21.1.Diaz, A.G. (1985).Magnetic generalization of the Kerr–Newman metric.JMP 26, 155.See §34.1.Dietz, W.(1983a).N rank zero HKX transformations, in Proceedings of the third MarcelGrossmann meeting on general relativity, ed.Hu Ning, page 1053 (North-Holland,Amsterdam).See §34.3.Dietz, W.(1983b).New representations of the HKX transformations by means ofdeterminants.GRG 15, 911.See §34.3.Dietz, W.(1984a).HKX transformations.Some results, in Solutions of Einstein’sequations: Techniques and results.Lecture notes in physics, vol.205, eds.C.Hoenselaers and W.Dietz, page 85 (Springer, Berlin).See §34.3.Dietz, W.(1984b).A new class of asymptotically flat stationary axisymmetric vacuumgravitational fields.GRG 16, 246.See §34.3.Dietz, W.(1988).New exact solutions of Einstein’s field equations: gravitational forcecan also be repulsive!Found. Phys. 18, 529.See §34.4.Dietz, W.and Hoenselaers, C.(1982a).A new class of bipolar vacuum gravitationalfields.Proc. Roy. Soc. London A 382, 221.See §34.3.Dietz, W.and Hoenselaers, C.(1982b). A new representation of the HKXtransformations.Phys.Lett. A 90, 218.See §34.3.Dietz, W.and Hoenselaers, C.(1982c).Stationary system of two masses kept apart bytheir gravitational spin-spin interaction.Phys. Rev. Lett. 48, 778.See §34.3.Dietz, W.and Hoenselaers, C.(1985).Two mass solutions of Einstein’s vacuumequations: the double Kerr solution.Ann. Phys. (USA) 165, 319.See §34.4.Dietz, W.and Rüdiger, R.(1981).Space-times admitting Killing Yano tensors I.Proc.Roy. Soc. Lond. A 375, 361.See §35.3.Dietz, W.and Rüdiger, R.(1982).Space-times admitting Killing Yano tensors II.Proc.Roy. Soc. Lond. A 381, 315.See §35.3.d’Inverno, R.A. and Russell-Clark, R.A. (1971). Classification of the Harrison metrics.JMP 12, 1258.See §§9.3, 17.3.Dodd, R.K., Kinoulty, J. and Morris, H.C. (1984). Bäcklund transformations forthe Ernst equation of general relativity, in Advances in nonlinear waves, ed.L.Debnath, page 254 (Pitman, Boston, MA).See §34.7.Dodd, R.K. and Morris, H.C. (1982). Linear deformation problems for the Ernstequation.JMP 23, 1131.See §34.7.Dodd, R.K. and Morris, H.C. (1983).Some equations that give special solutions to theErnst equation.Proc. Roy. Irish Acad. A 83, 95.See §20.6.Dolan, P.(1968).A singularity free solution of the Maxwell–Einstein-equation.Commun. Math. Phys. 9, 161.See §12.3.Dolan, P.and Kim, C.W.(1994).The wave equation for the Lanczos potential.I.Proc.Roy. Soc. London A 447, 557.See §3.6.Doroshkevich, A.G. (1965). Model of a universe with a uniform magnetic field (inRussian).Astrofiz. 1, 255.See §§14.1, 14.3.Doroshkevich, A.G., Lukash, V.N. and Novikov, I.D. (1973). Isotropisation ofhomogeneous cosmological models.Sov. Phys. JETP 37, 739.See §13.3.Dozmorov, I.M. (1971a).Solutions of the Einstein equations related by null vectors. II(in Russian).Izv. Vys. Uch. Zav. Fiz. 11, 68.See §32.5.

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