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Table 4.

Relative space motion among the various clouds of the Taurus complex.

Molecular cloud 1 Molecular cloud 2 Δu Δv Δw ΔVbulk Δd
(km s−1) (km s−1) (km s−1) (km s−1) (pc)
L 1517, L 1519 L 1544 3.0 ± 0.7 −2.4 ± 0.6 −1.4 ± 0.5 4.1 ± 0.7 20.1 ± 1.7
L 1517, L 1519 L 1495 1.5 ± 0.6 −2.6 ± 0.5 0.5 ± 0.4 3.0 ± 0.5 36.5 ± 1.2
L 1517, L 1519 B 213, B 216 3.3 ± 0.5 −1.5 ± 0.5 −3.3 ± 0.4 4.9 ± 0.5 22.7 ± 0.8
L 1517, L 1519 B 215 2.0 ± 0.8 −4.2 ± 0.7 −0.0 ± 0.6 4.7 ± 0.7 37.6 ± 2.0
L 1517, L 1519 Heiles Cloud 2 (cluster 14) 1.1 ± 0.6 −2.5 ± 0.5 −1.2 ± 0.4 3.0 ± 0.5 22.7 ± 1.7
L 1517, L 1519 Heiles Cloud 2 (cluster 15) 0.7 ± 0.6 −4.0 ± 0.5 −1.1 ± 0.4 4.2 ± 0.5 25.5 ± 1.7
L 1517, L 1519 L 1535, L 1529, L 1531, L 1524 1.5 ± 0.6 −3.6 ± 0.5 −0.8 ± 0.4 3.9 ± 0.5 36.3 ± 1.3
L 1517, L 1519 L 1536 1.8 ± 0.6 −0.8 ± 0.5 −3.4 ± 0.4 4.0 ± 0.5 24.7 ± 0.6
L 1517, L 1519 L 1551 1.1 ± 0.7 0.2 ± 0.5 −3.0 ± 0.5 3.2 ± 0.5 37.9 ± 0.8
L 1544 L 1495 −1.4 ± 0.6 −0.2 ± 0.4 1.9 ± 0.4 2.4 ± 0.4 50.9 ± 2.1
L 1544 B 213, B 216 0.4 ± 0.5 0.9 ± 0.5 −1.9 ± 0.4 2.1 ± 0.4 30.2 ± 1.7
L 1544 B 215 −1.0 ± 0.8 −1.8 ± 0.6 1.4 ± 0.5 2.5 ± 0.6 49.4 ± 2.8
L 1544 Heiles Cloud 2 (cluster 14) −1.8 ± 0.6 −0.1 ± 0.5 0.2 ± 0.4 1.8 ± 0.5 33.7 ± 2.6
L 1544 Heiles Cloud 2 (cluster 15) −2.2 ± 0.6 −1.6 ± 0.5 0.3 ± 0.4 2.7 ± 0.6 36.6 ± 2.6
L 1544 L 1535, L 1529, L 1531, L 1524 −1.5 ± 0.6 −1.2 ± 0.4 0.6 ± 0.3 2.0 ± 0.5 47.2 ± 2.3
L 1544 L 1536 −1.1 ± 0.6 1.6 ± 0.5 −2.0 ± 0.4 2.8 ± 0.5 24.0 ± 1.8
L 1544 L 1551 −1.9 ± 0.7 2.6 ± 0.5 −1.6 ± 0.4 3.6 ± 0.5 39.0 ± 1.9
L 1495 B 213, B 216 1.8 ± 0.3 1.0 ± 0.3 −3.8 ± 0.2 4.3 ± 0.2 30.9 ± 1.7
L 1495 B 215 0.5 ± 0.6 −1.7 ± 0.5 −0.5 ± 0.4 1.8 ± 0.5 7.9 ± 0.5
L 1495 Heiles Cloud 2 (cluster 14) −0.4 ± 0.3 0.1 ± 0.3 −1.7 ± 0.2 1.8 ± 0.2 17.8 ± 1.4
L 1495 Heiles Cloud 2 (cluster 15) −0.8 ± 0.5 −1.4 ± 0.3 −1.6 ± 0.2 2.3 ± 0.3 16.1 ± 1.1
L 1495 L 1535, L 1529, L 1531, L 1524 −0.0 ± 0.4 −1.0 ± 0.2 −1.3 ± 0.1 1.6 ± 0.2 11.9 ± 0.3
L 1495 L 1536 0.3 ± 0.4 1.7 ± 0.3 −4.0 ± 0.2 4.3 ± 0.2 35.3 ± 1.5
L 1495 L 1551 −0.4 ± 0.5 2.8 ± 0.3 −3.5 ± 0.3 4.5 ± 0.3 30.0 ± 0.5
B 213, B 216 B 215 −1.3 ± 0.6 −2.7 ± 0.5 3.2 ± 0.5 4.4 ± 0.5 32.0 ± 2.4
B 213, B 216 Heiles Cloud 2 (cluster 14) −2.2 ± 0.3 −1.0 ± 0.3 2.0 ± 0.2 3.1 ± 0.3 21.4 ± 1.8
B 213, B 216 Heiles Cloud 2 (cluster 15) −2.6 ± 0.4 −2.5 ± 0.3 2.2 ± 0.2 4.2 ± 0.3 25.1 ± 1.8
B 213, B 216 L 1535, L 1529, L 1531, L 1524 −1.8 ± 0.4 −2.1 ± 0.3 2.5 ± 0.2 3.7 ± 0.3 33.2 ± 1.7
B 213, B 216 L 1536 −1.5 ± 0.3 0.7 ± 0.3 −0.2 ± 0.3 1.6 ± 0.3 13.1 ± 0.8
B 213, B 216 L 1551 −2.2 ± 0.5 1.7 ± 0.3 0.3 ± 0.3 2.8 ± 0.4 28.7 ± 1.2
B 215 Heiles Cloud 2 (cluster 14) −0.9 ± 0.6 1.8 ± 0.5 −1.2 ± 0.5 2.3 ± 0.5 15.9 ± 2.4
B 215 Heiles Cloud 2 (cluster 15) −1.3 ± 0.7 0.2 ± 0.5 −1.0 ± 0.4 1.7 ± 0.6 13.3 ± 2.1
B 215 L 1535, L 1529, L 1531, L 1524 −0.5 ± 0.7 0.7 ± 0.5 −0.8 ± 0.4 1.1 ± 0.5 5.1 ± 0.6
B 215 L 1536 −0.2 ± 0.6 3.4 ± 0.5 −3.4 ± 0.5 4.8 ± 0.5 33.4 ± 2.3
B 215 L 1551 −0.9 ± 0.7 4.4 ± 0.5 −3.0 ± 0.5 5.4 ± 0.5 23.9 ± 1.2
Heiles Cloud 2 (cluster 14) Heiles Cloud 2 (cluster 15) −0.4 ± 0.4 −1.5 ± 0.3 0.1 ± 0.2 1.6 ± 0.3 3.9 ± 2.0
Heiles Cloud 2 (cluster 14) L 1535, L 1529, L 1531, L 1524 0.3 ± 0.4 −1.1 ± 0.3 0.4 ± 0.2 1.2 ± 0.3 14.4 ± 1.8
Heiles Cloud 2 (cluster 14) L 1536 0.7 ± 0.4 1.7 ± 0.3 −2.2 ± 0.3 2.9 ± 0.3 21.2 ± 1.8
Heiles Cloud 2 (cluster 14) L 1551 −0.1 ± 0.5 2.7 ± 0.4 −1.8 ± 0.3 3.2 ± 0.3 20.5 ± 0.5
Heiles Cloud 2 (cluster 15) L 1535, L 1529, L 1531, L 1524 0.7 ± 0.5 0.4 ± 0.3 0.3 ± 0.1 0.9 ± 0.5 11.0 ± 1.6
Heiles Cloud 2 (cluster 15) L 1536 1.1 ± 0.5 3.2 ± 0.3 −2.4 ± 0.2 4.1 ± 0.3 24.6 ± 1.8
Heiles Cloud 2 (cluster 15) L 1551 0.3 ± 0.6 4.2 ± 0.4 −1.9 ± 0.3 4.6 ± 0.3 20.9 ± 0.5
L 1535, L 1529, L 1531, L 1524 L 1536 0.4 ± 0.5 2.7 ± 0.3 −2.7 ± 0.2 3.8 ± 0.3 33.0 ± 1.6
L 1535, L 1529, L 1531, L 1524 L 1551 −0.4 ± 0.6 3.8 ± 0.3 −2.2 ± 0.3 4.4 ± 0.3 22.6 ± 0.6
L 1536 L 1551 −0.8 ± 0.5 1.0 ± 0.4 0.5 ± 0.3 1.4 ± 0.4 20.8 ± 1.4

Notes. We provide the relative motion for each component of the spatial velocity (in the sense molecular cloud 1 minus molecular cloud 2), the resulting bulk motion between the clouds, and their relative distance computed from the XYZ coordinates of the cloud centers (see Table 2).

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