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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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