Table 2
Accretion rates onto the binary and mass fluxes F in units M / P0 × 10-5 at two selected distances to the binary CoM: r1 = a and r2 = 1.5 a.
| r1 = a | r2 = 1.5a | ||||||||
|
|
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| Model | Ṁ 1 | Ṁ 2 | Ṁ | F in1 | F out1 | F net1 | F in2 | F out2 | F net2 |
|
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| iso10 | 4.5 | 10.7 | 15.2 | 19.6 | 4.5 | 15.1 | 33.7 | 18.8 | 14.9 |
| iso05 | 4.2 | 9.2 | 13.4 | 19.1 | 5.5 | 13.6 | 31.7 | 18.4 | 13.4 |
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| adia10 | 3.8 | 9.5 | 13.3 | 17.6 | 4.3 | 13.3 | 42.8 | 29.7 | 13.2 |
| adia05 | 3.2 | 4.6 | 7.8 | 13.5 | 5.8 | 7.7 | 36.0 | 28.4 | 7.6 |
Notes. Ṁ1 and Ṁ2 are the average accretion rates on M1 and M2 respectively, while Ṁ is the sum of the two. At both selected distances, Fin and Fout represent the ingoing and outgoing fluxes, and Fnet = Fin − Fout is the net ingoing flux. All quantities have been averaged over 90 binary orbits.
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