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Comments on the comment on the Guzman-Bianchi type-VII h solutions

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Abstract

In this paper, we again discuss the new Brans-Dicke-Bianchi type-VII h perfect fluid solutions, first given by us (Guzman, 1989). It is shown that the objections presented by Lorenz-Petzold (1989) are misleading. The dust case β=0 is discussed.

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References

  • Chauvet, P. and Guzman, E.: 1986,Astrophys. Space Sci. 126, 133.

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  • Guzman, E.: 1989,Astrophys. Space Sci. 152, 171.

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  • Lorenz-Petzold, D.: 1984,Astrophys. Space Sci. 106, 409.

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  • Lorenz-Petzold, D.: 1989,Astrophys. Space Sci. 161, 163.

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  • Zel'dovich, Ya. B. and Novikov, I. D.: 1983,Relativistic Astrophysics, Vol. 2, Chicago Press, Chicago.

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Authors and Affiliations

  1. Astronomisches Institut, Ruhr-Universität, Bochum, FRG

    Enrique Guzman

  2. Universidad Autonoma Metropolitana-Iztapalapa, Mexico, D.F.

    Enrique Guzman

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  1. Enrique Guzman
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Guzman, E. Comments on the comment on the Guzman-Bianchi type-VII h solutions. Astrophys Space Sci 173, 163–164 (1990). https://doi.org/10.1007/BF00642571

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  • DOI: https://doi.org/10.1007/BF00642571

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