Table 3.
Spatial velocity of the Taurus molecular clouds.
Molecular Cloud | Cluster | N | U | V | W | Vspace | ||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(km s−1) |
(km s−1) |
(km s−1) |
(km s−1) |
|||||||||||
Mean ± SEM | Median | SD | Mean ± SEM | Median | SD | Mean ± SEM | Median | SD | Mean ± SEM | Median | SD | |||
L 1517, L 1519 | 1 | 2 | −14.6 ± 0.1 | −14.6 | 0.8 | −14.7 ± 0.3 | −14.7 | 0.0 | −10.3 ± 0.3 | −10.3 | 0.2 | 23.2 ± 0.4 | 23.2 | 0.5 |
L 1544 | 4 | 2 | −17.6 ± 0.1 | −17.6 | 0.4 | −12.3 ± 0.2 | −12.3 | 0.9 | −8.9 ± 0.2 | −8.9 | 0.3 | 23.2 ± 0.3 | 23.2 | 0.7 |
L 1495 NW | 6 | 0 | ||||||||||||
L 1495 | 7 | 25 | −16.1 ± 0.2 | −15.9 | 1.1 | −12.2 ± 0.2 | −12.2 | 0.8 | −10.8 ± 0.1 | −10.8 | 0.5 | 23.0 ± 0.2 | 22.9 | 0.9 |
B 213, B 216 | 8 | 8 | −17.9 ± 0.2 | −18.0 | 0.5 | −13.2 ± 0.2 | −13.3 | 0.6 | −7.0 ± 0.2 | −7.1 | 0.5 | 23.4 ± 0.2 | 23.4 | 0.4 |
B 215 | 9 | 2 | −16.6 ± 0.2 | −16.6 | 0.3 | −10.5 ± 0.3 | −10.5 | 0.0 | −10.3 ± 0.3 | −10.3 | 0.0 | 22.2 ± 0.5 | 22.2 | 0.2 |
Heiles Cloud 2 | 14 | 3 | −15.7 ± 0.2 | −15.6 | 0.4 | −12.3 ± 0.2 | −12.4 | 0.4 | −9.1 ± 0.2 | −9.0 | 0.3 | 21.9 ± 0.2 | 21.8 | 0.3 |
Heiles Cloud 2 | 15 | 5 | −15.4 ± 0.4 | −15.4 | 0.9 | −10.8 ± 0.2 | −10.5 | 0.5 | −9.2 ± 0.1 | −9.3 | 0.3 | 20.9 ± 0.3 | 20.9 | 0.7 |
L 1535, L 1529, L 1531, L 1524 | 16 | 10 | −16.1 ± 0.3 | −15.9 | 1.1 | −11.2 ± 0.2 | −11.1 | 0.5 | −9.5 ± 0.1 | −9.6 | 0.2 | 21.8 ± 0.2 | 21.7 | 0.8 |
L 1536 | 18 | 14 | −16.4 ± 0.3 | −16.4 | 1.1 | −13.9 ± 0.3 | −13.7 | 0.9 | −6.8 ± 0.2 | −6.9 | 0.8 | 22.6 ± 0.2 | 22.3 | 0.9 |
T Tau cloud | 19 | 1 | −18.0 ± 0.2 | −18.0 | −8.0 ± 0.6 | −8.0 | −8.0 ± 0.6 | −8.0 | 21.3 ± 0.6 | 21.3 | ||||
L 1551 | 20 | 12 | −15.7 ± 0.5 | −16.1 | 1.6 | −15.0 ± 0.3 | −14.9 | 0.9 | −7.3 ± 0.3 | −7.5 | 0.9 | 22.9 ± 0.5 | 23.6 | 1.6 |
L 1558 | 21 | 0 | ||||||||||||
Taurus (complex) | All | 92 | −16.2 ± 0.1 | −16.2 | 1.3 | −12.8 ± 0.2 | −12.7 | 1.6 | −8.9 ± 0.2 | −9.0 | 1.7 | 22.5 ± 0.1 | 22.6 | 1.2 |
Notes. We provide for each cloud its identifier, corresponding cluster in the HMAC analysis (see Sect. 4), number of stars with measured radial velocity, mean, standard error of the mean (SEM), median, and standard deviation of the Galactic UVW velocity components (not corrected for the solar motion). The standard deviation value given in the table represents the difference between the individual measurements when the molecular cloud has only two representative stars.
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