Table 1
Cores included in the GEMS sample and observation cuts associated with them.
| Cloud complex | Cloud | Core | Coordinates | Other names | Cut | No | Nv | |
|---|---|---|---|---|---|---|---|---|
| ID | RA (J2000) | Dec (J2000) | ||||||
| Taurus | TMC 1 | CP | 04:41:41.90 | +25:41:27.1 | C1 | 6 | 6 | |
| NH3 | 04:41:21.30 | +25:48:07.0 | C2 | 6 | 6 | |||
| C | 04:41:38.80 | +25:59:42.0 | C3 | 6 | 6 | |||
| B 213-N(1) | #1 | 04:17:41.80 | +28:08:47.0 | 5 | C1 | 9 | 9 | |
| #2 | 04:17:50.60 | +27:56:01.0 | – | C2 | 9 | 7 | ||
| #5 | 04:18:03.80 | +28:23:06.0 | 7 | C5 | 9 | 9 | ||
| #6 | 04:18:08.40 | +28:05:12.0 | 8 | C6 | 9 | 5 | ||
| #7 | 04:18:11.50 | +27:35:15.0 | 9 | C7 | 9 | 8 | ||
| B213-S(1) | #10 | 04:19:37.60 | +27:15:31.0 | 13a | C10 | 9 | 8 | |
| #12 | 04:19:51.70 | +27:11:33.0 | – | C12 | 9 | 6 | ||
| #16 | 04:21:21.00 | +27:00:09.0 | – | C16 | 9 | 9 | ||
| #17 | 04:27:54.00 | +26:17:50.0 | 26b | C17 | 9 | 5 | ||
| Perseus | L1448(2) | #32 | 03:25:49.00 | +30:42:24.6 | C1 | 8 | 7 | |
| NGC1333(2) | 03:29:18.26 | +31:28:02.0 | C1 | 21 | 18 | |||
| 03:28:41.60 | +31:06:02.0 | C2 | 17 | 13 | ||||
| #46 | 03:29:11.00 | +31:18:27.4 | SK20(3) | C3 | 17 | 11 | ||
| #60 | 03:28:39.40 | +31:18:27.4 | ||||||
| #51 | 03:29:08.80 | +31:15:18.1 | SK16 | C4 | 16 | 13 | ||
| #53 | 03:29:04.50 | +31:20:59.1 | SK26 | C5 | 11 | 11 | ||
| #57 | 03:29:18.20 | +31:25:10.8 | SK33 | C6 | 9 | 9 | ||
| #64 | 03:29:25.50 | +31:28:18.1 | C7 | 1 | 1 | |||
| Barnard 1(2) | 1b | 03:33:20.80 | +31:07:34.0 | C1 | 18 | 18 | ||
| 03:33:01.90 | +31:04:23.2 | C2 | 8 | 6 | ||||
| Barnard 5(2) | #79 | 03:47:38.99 | +32:52:15.0 | C1 | 13 | 9 | ||
| IC 348(2) | #1 | 03:44:01.00 | +32:01:54.8 | C1 | 14 | 11 | ||
| #10 | 03:44:05.74 | +32:01:53.5 | ||||||
| Orion | Orion A | OMC 3 | 05:35:19.54 | −05:00:41.5 | C1 | 20 | 10 | |
| OMC 4 | 05:35:08.15 | −05:35:41.5 | C2 | 20 | 14 | |||
| OMC 2 | 05:35:23.68 | −05:12:31.8 | C3 | 13 | 9 | |||
| TOTAL | 305 | 244 | ||||||
Notes. No indicates the total number of points observed in the corresponding cut. Nv indicates the number of points where the molecular hydrogen density could be derived. (1)B 213 core IDs are from Hacar et al. (2013). IDs indicated in “Other names” column are from Onishi et al. (2002). (2)Perseus core IDs (L 1448, NGC 1333, Barnard 1, Barnard 5, IC348) are from Hatchell et al. (2007b). (3)NGC 1333 core IDs indicated in “Other names” column are from Sandell & Knee (2001).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.