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Table A.2
Coefficients of the fourth-order polynomial fits (Eq. (A.2)) to the variation of each of the six parameters (Mi/Md and ai/Rd) as a function of b/Rd for the modelling of the thin stellar disk based on the three MN-disks model shown in Fig. A.2.
| Parameter | c0 | c1 | c2 | c3 | c4 |
|
|
|||||
| M1/Md | 0.8211 | 0.3237 | −1.0203 | 1.1239 | −0.2535 |
| M2/Md | 0.8887 | −0.2588 | 0.8416 | −1.2136 | 0.4836 |
| M3/Md | −0.7007 | 0.1463 | −0.0123 | 0.0789 | −0.1921 |
| a1/Rd | 1.8576 | −0.8626 | 0.8327 | −1.3109 | 0.6661 |
| a2/Rd | 3.9650 | 2.1244 | -4.3408 | 3.4060 | −1.4135 |
| a3/Rd | 1.5509 | −1.3112 | 2.0039 | −3.2060 | 1.3294 |
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