The maximum initial orbital period (in hours) of two point masses that will coalesce due to gravitational wave emission in a time interval shorter than 1010 yr, as a function of the initial eccentricity e0. The lines are calculated for 10 M⊙ + 10 M⊙ (BH + BH), 10 M⊙ + 1.4 M⊙ (BH + NS), and 1.4 M⊙ +1.4 M⊙ (NS + NS).
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