Table 6
New Galactocentric 
and heliocentric (d) distances computed from the peak velocity (Vp) of the c-C3H2 
= 21,2-10,1 line as explained in Sect. 4.3.
| Source | Longitude deg |
 kms-1 |
 kpc |
d kpc |
|---|---|---|---|---|
| WB89-315 | 118.0 | –95.1(0.3)(b) | 16.3 | 10.7 |
| WB89-379 | 124.6 | –89.16(0.06) | 16.4 | 10.2 |
| WB89-380 | 124.6 | –86.68(0.04) | 16.0 | 9.7 |
| WB89-391 | 125.8 | –86.10(0.02) | 16.1 | 9.7 |
| WB89-399 | 128.8 | –82.15(0.05) | 16.0 | 9.4 |
| WB89-437 | 135.3 | –72.14(0.06) | 15.7 | 8.6 |
| WB89-440 | 135.6 | –71.88(0.05) | 15.7 | 8.6 |
| WB89-501 | 145.2 | –58.43(0.04) | 15.6 | 8.0 |
| WB89-529 | 149.6 | –59.8(0.2) | 17.8 | 10.1 |
| WB89-572 | 156.9 | –47.4(0.1) | 18.3 | 10.3 |
| WB89-621 | 168.1 | –25.68(0.07) | 18.9 | 10.6 |
| WB89-640 | 167.1 | –24.93(0.08) | 16.8 | 8.6 |
| WB89-670 | 173.0 | –17.65(0.01) | 23.4 | 15.1 |
| WB89-705 | 174.7 | –12.20(0.01) | 20.5 | 12.2 |
| WB89-789 | 195.8 | 34.25(0.05) | 19.1 | 11.0 |
| WB89-793 | 195.8 | 30.5(0.2) | 16.9 | 8.7 |
| WB89-898 | 217.6 | 63.5(0.1) | 15.8 | 8.4 |
| 19423+2541 | 61.72 | –72.58(0.04) | 13.5 | 15.3 |
| 19383+2711 | 62.58 | –70.2(0.2) | 13.2 | 14.8 |
| 19383+2711-b(c) | 62.58 | –65.6(0.2) | 12.7 | 14.2 |
| 19489+3030 | 66.61 | –69.29(0.05) | 12.9 | 13.7 |
| 19571+3113 | 68.15 | –61.7(0.1) | 12.2 | 12.5 |
| 19571+3113-b(c) | 68.15 | –66.2(0.1) | 12.5 | 13.0 |
| 20243+3853 | 77.6 | –73.21(0.05) | 12.8 | 11.7 |
| WB89-002 | 85.41 | –2.83(0.09) | 8.65 | 3.1 |
| WB89-006 | 86.27 | –90.38(0.05) | 14.3 | 12.2 |
| WB89-014 | 88.99 | –96.0(0.1) | 14.9 | 12.5 |
| WB89-031 | 88.06 | –88.89(0.08) | 14.1 | 11.7 |
| WB89-035 | 89.94 | –77.56(0.03) | 13.1 | 10.1 |
| WB89-040 | 90.68 | –62.38(0.05) | 11.9 | 8.3 |
| WB89-060 | 95.05 | –83.7(0.15) | 13.6 | 10.1 |
| WB89-076 | 95.25 | –97.07(0.02) | 15.1 | 11.8 |
| WB89-080 | 95.44 | –74.1(0.2) | 12.8 | 8.9 |
| WB89-083 | 96.08 | –93.76(0.04) | 14.7 | 11.2 |
| WB89-152 | 104.0 | –88.5(0.2) | 14.4 | 9.8 |
| WB89-283 | 114.3 | –94.69(0.06) | 15.8 | 10.4 |
| WB89-288 | 114.3 | –101.0(0.1) | 16.8 | 11.5 |
Notes. (a)Obtained from the Gaussian fits in Table B.2. Uncertainties derived from the fitting procedure are provided in parentheses. (b)Source undetected in c-C3H2 and in any other optically thin transition (Table 3). We use the VLSR given in Blair et al. (2008).(c)Second velocity feature (see Fig. B.2).
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