Table 1
Evolution rates calculated numerically, (drp/ dt)n, and analytically as indicated above, (drp/ dt)a, for different values of the mass ratio q.
q | (drp/ dt)n | (drp/ dt)a |
|
||
0.0001 | –2.1e-6 | –2.8e-6 |
0.0005 | –1.6e-5 | –1.4e-5 |
0.001 | –3.4e-5 | –2.8e-5 |
0.003 | –7.9e-5 | –8.3e-5 |
Notes. The evolution rates, time-averaged over several orbits and evaluated at early times, are in units , where P0 is the initial orbital period of the perturber. The softening length for these calculations was taken to be 0.6H.
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