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Figure 10: Cross section of equipotential surfaces in the orbital plane of a binary with q = 0.4.
The values of the potential surfaces are 5.0, 3.9075, 3.8, 3.559, 3.2, 3.0, and 2.8. The units have been
normalized to the orbital separation, so a = 1.
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Matthew J. Benacquista and Jonathan M. B. Downing, "Relativistic Binaries in Globular Clusters",
Living Rev. Relativity, 16 (2013), 4, doi:10.12942/lrr-2013-4, URL (accessed <date>): http://www.livingreviews.org/lrr-2013-4.
This work is licensed under a Creative Commons License.
© The author(s), except where otherwise noted.
Living Rev. Relativity, 16 (2013), 4, doi:10.12942/lrr-2013-4, URL (accessed <date>): http://www.livingreviews.org/lrr-2013-4.
This work is licensed under a Creative Commons License.
© The author(s), except where otherwise noted.