Table 4.
Lines marked in Fig. 6.
| n. | Name | Arch | Group | Points | Slope | r |
|---|---|---|---|---|---|---|
| L1 | G42 | 4 | −9.0 ± 2.1 | −0.95 | ||
| L2 | Arch 1 | A1 | G19 | 3 | 25.0 ± 0.0 | 1.00 |
| L3 | Sirius | A4 | G3 | 32 | 19.2 ± 0.4 | 0.99 |
| L4 | Coma Berenices | A5 | G4 | 4 | 13.0 ± 0.7 | 1.00 |
| L5 | Hyades | A7 | G1 | 20 | 24.9 ± 0.5 | 1.00 |
| L6 | 4 | 33.5 ± 0.9 | 1.00 | |||
| L7 | Dehnen98-6 | A5 | G7 | 9 | 13.3 ± 2.2 | 0.92 |
| L8 | Dehnen98-14 | A6 | G6 | 16 | 20.0 ± 0.7 | 0.99 |
| L9 | Hercules II | A9 | G5 | 15 | 26.5 ± 0.2 | 1.00 |
| L10 | Liang17-9 | A9 | G10 | 15 | 14.3 ± 0.5 | 0.99 |
| L11 | HR 1614 | A10 | G13 | 4 | 19.0 ± 2.1 | 0.99 |
| L12 | Bobylev16-22 | A11 | G16 | 5 | 31.0 ± 2.7 | 0.99 |
| L13a | Arcturus | A12 | 7 | 29.8 ± 1.5 | 0.99 | |
| L13b | Arcturus | A12 | 5 | 32.9 ± 3.4 | 0.98 | |
| L14 | 8 | 30.2 ± 5.2 | 0.92 | |||
| L15 | 5 | 22.5 ± 1.7 | 0.99 | |||
| L16 | 20 | 22.0 ± 0.4 | 1.00 | |||
| L17 | 24 | 23.4 ± 0.8 | 0.99 | |||
| L18 | 12 | 31.0 ± 1.8 | 0.98 | |||
| L19 | 5 | 6.0 ± 1.9 | 0.88 | |||
| L20 | 5 | 32.0 ± 1.2 | 1.00 | |||
| L21 | 4 | −14.0 ± 5.9 | −0.86 | |||
| L22 | 6 | −8.5 ± 2.5 | −0.86 | |||
| L23 | 8 | 31.4 ± 2.0 | 0.99 | |||
| L24 | 11 | 10.0 ± 1.3 | 0.93 | |||
| L25 | 8 | 7.9 ± 1.2 | 0.92 | |||
| L26 | 6 | −20.4 ± 6.8 | −0.83 |
Notes. The first column contains the label of the Line, while the second refers to the name of the structure at Solar radius (if possible). Subsequently, Cols. 3 and 4 contain the Arches (Table 2) and Groups (Table 3) corresponding to the peak at Solar radius of the Line. The last three columns characterise the lines by, respectively, their number of points, the slope (km s−1 kpc−1) obtained from the linear regression and the corresponding correlation coefficient, r.
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