Table 1
Source parameters extracted from Table 1 of Blair et al. (2008).
| Source | RA (J2000) |
Dec (J2000) |
VLSR(1) kms-1 |
N (H2)(2) ×1021 cm-2 |
 kpc |
M(4) M⊕ | L(4) (×103) L⊕ |
|---|---|---|---|---|---|---|---|
| WB89-315 | 00:05:53.8 | 64:05:17 | –95.09 | 3.7 | 17.1 | ||
| WB89-379 | 01:06:59.9 | 65:20:51 | –89.32 | 6.5 | 17.3 | 532 | 1.44 |
| WB89-380 | 01:07:50.9 | 65:21:22 | –86.67 | 11.4 | 17.0 | ||
| WB89-391 | 01:19:27.1 | 65:45:44 | –86.06 | 5.2 | 16.9 | ||
| WB89-399 | 01:45:39.4 | 64:16:00 | –82.19 | 6.3 | 16.8 | 1685 | 16.3 |
| WB89-437 | 02:43:29.0 | 62:57:08 | –71.72 | 14.2 | 16.2 | ||
| WB89-440 | 02:46:07.3 | 62:46:31 | –72.20 | 4.1 | 16.4 | ||
| WB89-501 | 03:52:27.6 | 57:48:34 | –58.44 | 11.2 | 16.4 | ||
| WB89-529 | 04:06:25.5 | 53:21:49 | –60.08 | 4.7 | 17.8 | 408 | 10.1 |
| WB89-572 | 04:35:58.3 | 47:42:58 | –48.03 | 3.8 | 20.4 | ||
| WB89-621 | 05:17:13.4 | 39:22:15 | –25.38 | 13.0 | 22.6 | 920 | 41.2 |
| WB89-640 | 05:25:40.7 | 41:41:53 | –25.42 | 3.2 | 18.4 | ||
| WB89-670 | 05:37:41.9 | 36:07:22 | –17.52 | 7.3 | 23.5 | ||
| WB89-705 | 05:47:47.6 | 35:22:01 | –12.10 | 1.7 | 21.4 | ||
| WB89-789 | 06:17:24.3 | 14:54:37 | 34.33 | 5.8 | 20.3 | 1066 | 9.75 |
| WB89-793 | 06:18:41.7 | 15:04:52 | 30.48 | 5.9 | 18.1 | 204 | 0.77 |
| WB89-898 | 06:50:37.3 | -05:21:01 | 63.41 | 2.5 | 16.4 | ||
| 19383+2711 | 19:40:22.1 | 27:18:33 | –66.85 | – | 13.2 | ||
| 19423+2541 | 19:44:23.2 | 25:48:40 | –72.62 | – | 13.6 | 1278 | 104.5 |
| 19489+3030 | 19:50:53.2 | 30:38:09 | –68.91 | – | 13.0 | ||
| 19571+3113 | 19:59:08.5 | 31:21:47 | –62.48 | – | 12.2 | ||
| 20243+3853 | 20:26:10.8 | 39:03:30 | –73.06 | – | 12.9 | 891 | 15.9 |
| WB89-002 | 20:37:22.3 | 47:13:54 | –2.75 | 7.8 | 8.6 | ||
| WB89-006 | 20:42:58.2 | 47:35:35 | –91.38 | 6.3 | 14.9 | ||
| WB89-014 | 20:52:07.8 | 49:51:28 | –96.03 | 4.6 | 15.5 | ||
| WB89-031 | 21:04:18.0 | 46:53:10 | –89.40 | 1.2 | 14.6 | ||
| WB89-035 | 21:05:19.7 | 49:15:59 | –77.68 | 5.2 | 13.4 | 367 | 5.23 |
| WB89-040 | 21:06:50.0 | 50:02:09 | –62.65 | 4.1 | 12.1 | 613 | 0.62 |
| WB89-060 | 21:15:56.0 | 54:43:33 | –84.29 | 9.3 | 14.0 | ||
| WB89-076 | 21:24:29.0 | 53:45:35 | –97.17 | 5.0 | 15.7 | 355 | 0.82 |
| WB89-080 | 21:26:29.1 | 53:44:11 | –74.24 | 8.5 | 13.1 | 299 | 1.44 |
| WB89-083 | 21:27:47.7 | 54:26:58 | –93.77 | 2.8 | 15.3 | 220 | 0.82 |
| WB89-152 | 22:05:15.4 | 60:48:41 | –88.13 | 2.8 | 14.8 | ||
| WB89-283 | 23:32:23.8 | 63:33:18 | –94.49 | 5.8 | 16.5 | 140 | 4.80 |
| WB89-288 | 23:36:08.1 | 62:23:48 | –100.87 | 3.4 | 17.5 | 373 | 3.22 |
Notes. (1)Local standard of rest velocities used to centre the spectra; (2)H2 column densities from CO (1–0) (Blair et al. 2008), assuming a standard CO-H2 conversion factor of 1.8 × 1020 cm-2 (Kkms-1)-1 (Dame et al. 2001), which is valid at the Solar circle. The values were averaged within the Arizona Radio Observatory (ARO) main beam of 44″; (3)Galactocentric distances based on the rotation curve of Brand & Blitz (1993). We derive updated values for RGC in Sect. 4.3; (4)total gas mass, M, and bolometric luminosity, L, respectively, derived from Herschel measurements by Elia et al. (2021), and rescaled when needed to the new heliocentric distances calculated in this work (Table 6).
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