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Table 3
Angular distance to the central star of all points on the "Wilkinoid" that fall in the aperture when projected on the sky for various inclination angles (i) based on the Wilkin model, and the derived distance to CW Leo.
| i | Δθ | distance | i | Δθ | distance |
| (°) | (′′) | (pc) | (°) | (′′) | (pc) |
|
|
|||||
| 0 | 534.4 ± 18.3 | 130.2 ± 12.7 | 33.3 | 564.7 ± 37.4 | 123.3 ± 13.7 |
| 10 | 540.9 ± 19.8 | 128.6 ± 12.7 | 36 | 568.1 ± 39.0 | 122.5 ± 13.7 |
| 20 | 550.5 ± 25.6 | 126.4 ± 12.9 | 50 | 600.6 ± 56.0 | 115.9 ± 14.5 |
| 30 | 561.2 ± 30.4 | 124.0 ± 13.1 | 60 | 655.7 ± 77.0 | 106.1 ± 14.8 |
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