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AbstractAbstract
[en] This paper attempts a definitive treatment of ''classical gravitational bremsstrahlung''--i.e., of the gravitational waves produced when two stars of arbitrary relative mass fly past each other with arbitrary relative velocity v, but with large enough impact parameter that (angle of gravitational deflection of stars' orbits) very-much-less-than (1-v2/c2)/sup 1/2/
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Journal Article
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Astrophysical Journal; v. 224(1); p. 62-85
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