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Table C.1
Kinematic Galactocentric and heliocentric distances derived from the rotation curve of Reid et al. (2019).
| Source |  kpc |
d(1) kpc |
|---|---|---|
| WB89-315 | 14.63 | 8.72 |
| WB89-379 | 14.66 | 8.21 |
| WB89-380 | 14.35 | 7.86 |
| WB89-391 | 14.43 | 7.86 |
| WB89-399 | 14.34 | 7.55 |
| WB89-437 | 14.02 | 6.79 |
| WB89-440 | 14.04 | 6.80 |
| WB89-501 | 13.92 | 6.22 |
| WB89-529 | 15.58 | 7.79 |
| WB89-572 | 15.74 | 7.71 |
| WB89-621 | 15.44 | 7.17 |
| WB89-640 | 14.1 | 5.84 |
| WB89-670 | 17.04 | 8.72 |
| WB89-705 | 14.63 | 6.30 |
| WB89-789 | 18.66 | 10.49 |
| WB89-793 | 16.57 | 8.38 |
| WB89-898 | 14.93 | 7.42 |
| 19423+2541 | 12.13 | 13.60 |
| 19383+2711 | 12.28 | 13.63 |
| 19489+3030 | 11.84 | 12.34 |
| 19571+3113 | 11.26 | 11.27 |
| 20243+3853 | 11.84 | 10.37 |
| WB89-002 | 8.369 | 1.54 |
| WB89-006 | 13.02 | 10.55 |
| WB89-014 | 13.49 | 10.74 |
| WB89-031 | 12.91 | 10.13 |
| WB89-035 | 12.03 | 8.67 |
| WB89-040 | 11.04 | 7.12 |
| WB89-060 | 12.5 | 8.59 |
| WB89-076 | 13.64 | 10.05 |
| WB89-080 | 11.81 | 7.60 |
| WB89-083 | 13.35 | 9.57 |
| WB89-152 | 13.07 | 8.24 |
| WB89-283 | 14.24 | 8.60 |
| WB89-288 | 14.98 | 9.47 |
(1) We adopted the same longitude and Vp (for sources having two velocity features, only the main one is used) as in Table 6.
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