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Gravitational radiation and spiralling time of close binary systems

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Abstract

Power-output by gravitational radiation (P B ) and spiral time (τ0) for individual systems of sixteen eclipsing binary stars have been evaluated, and a relation betweenP B and τ0 obtained.

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References

  • Giannone, P. and Giannuzzi, M. A.: 1974,Astrophys. Space Sci. 26, 289.

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  • Parker, Sybil P.: 1983,McGraw-Hill Encyclopedia of Astronomy, New York, p. 136.

  • Srivastava, R. K. and Padalia, T. D.: 1975,Astrophys. Space Sci. 38, 79.

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Authors and Affiliations

  1. Uttar Pradesh State Observatory, Naini Tal, India

    T. D. Padalia

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  1. T. D. Padalia
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Padalia, T.D. Gravitational radiation and spiralling time of close binary systems. Astrophys Space Sci 137, 191–194 (1987). https://doi.org/10.1007/BF00641633

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  • DOI: https://doi.org/10.1007/BF00641633

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