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Fig. 2
Spectra of the GW radiation from a long-living binary (M1 = M2 = 300 M⊙, a = 1.2 × 106 R⊙) for different values of eccentricity. A single “plus” mark corresponds to a circular orbit, by crosses we show the case for eccentricity 0.5, stars corresponds to eccentricity 0.7, and squares to initial eccentricity 0.9.
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