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Table 3

Kinematic differences when comparing positive and negative Galactic longitudes in the spiral models.

1 2 3 4 5 6 7 8 9 10 11 12 13

Model l max D max (Δ−Δexp)max l l %≥ 2 km s-1 %≥ 5 km s-1 | Δ−Δexp | med U U(l = [ 155,175 ] °)
(°) ( kpc) ( km s-1) (°) ( km s-1) (°) ( km s-1) ( km s-1) ( km s-1) ( km s-1)

TWA0 15 3.8 22.9 ±0.3 75 11.4 175 0.3 68 53 5.5 12.6 ±0.4 9.3 ±0.7
TWA1 15 4.8 12.2 ±0.3 75 4.1 175 0.2 49 7 1.9 10.1 ±0.2 9.1 ±0.3
TWA2 5 5.8 –10.0 ±0.3 35 2.2 175 0.3 13 0 0.9 9.1 ±0.1 9.5 ±0.2
TWA3 25 4.8 8.9 ±0.3 25 4.2 175 0.4 50 6 2.1 8.6 ±0.2 8.9 ±0.4
TWA10 15 4.8 8.7 ±0.5 25 3.4 165 0.5 29 3 1.4 9.5 ±0.1 9.5 ±0.3
TWA11 15 4.8 5.6 ±0.3 75 2.1 165 0.3 16 0 0.8 9.3 ±0.1 9.1 ±0.2
TWA12 15 4.8 14.8 ±0.3 75 7.2 175 0.3 61 36 3.2 11.0 ±0.3 8.9 ±0.5
TWA13 15 4.8 15.5 ±0.5 75 7.9 175 0.4 57 27 2.6 10.1 ±0.4 8.8 ±0.4
B1 145 0.2 –73.5 ±37.0 95 34.5 35 3.4 86 70 9.9 1.1 ±0.9 –2.8 ±3.1
B5 135 4.8 91.4 ±1.5 135 37.2 175 7.5 94 86 15.7 14.2 ±1.7 39.9 ±3.1
U5 95 5.2 –14.7 ±0.9 95 9.9 175 1.1 67 36 3.6 6.6 ±0.2 6.7 ±0.6
U5b 55 0.2 12.6 ±3.8 55 6.9 175 1.6 60 22 2.7 9.7 ±0.3 8.8 ±0.8

Notes. Columns show: 2)–4) Galactic longitude with the bin of maximum | Δ−Δexp | in the explored range of distances (6 kpc), distance of this bin, and corresponding value of Δ−Δexp; 5) and 6) longitude of maximum mean | Δ−Δexp | and corresponding maximum mean | Δ−Δexp | for this longitude; 7) and 8) longitudes of minimum mean | Δ−Δexp | and corresponding minimum mean; 9) fraction of bins with | Δ−Δexp | ≥ 2 km s-1; 10) fraction of bins with | Δ−Δexp | ≥ 5 km s-1; 11) median value of | Δ−Δexp |; 12) derived value of U from Eq. (2) obtained through a median (see text); 13) same as 12) but only for bins at l = 155°, 165°, 175 °.

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