Table 2
New GLIMPSE stellar clusters identified in this work.
| G3CC | ℓ | b | α | δ | Diam. | N circ | Det. | Flags |
| (°) | (°) | (J2000) | (J2000) | (″) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
||||||||
| 1 | 295.151 | −0.587 | 11:43:24.9 | −62:25:36 | 98 | 16 | A | C8, E8, S |
| 2 | 299.014 | 0.128 | 12:17:24.9 | −62:29:04 | 60 | 4 | V | B, E8 |
| 3 | 299.051 | 0.181 | 12:17:47.9 | −62:26:12 | 81 | 14 | A | C8 |
| 4a | 299.337 | −0.319 | 12:19:43.1 | −62:58:08 | 51 | 9 | A | BR,E8 |
| 5 | 300.913 | 0.887 | 12:34:16.2 | −61:55:04 | 76 | 10 | A | C8, E8 |
| 6 | 301.643 | −0.240 | 12:40:02.6 | −63:05:01 | 67 | 9 | A | DC, E8, S |
| 7 | 301.947 | 0.313 | 12:42:53.7 | −62:32:32 | 65 | 12 | A | E8 |
| 8 | 303.927 | −0.687 | 13:00:22.2 | −63:32:30 | 107 | 14 | A | C8, E8 |
| 9 | 304.002 | 0.464 | 13:00:40.3 | −62:23:17 | 82 | ··· | A | BR, E8, S |
| 10 | 304.887 | 0.635 | 13:08:12.3 | −62:10:23 | 41 | 7 | A | DC, E4 |
| 11 | 307.083 | 0.528 | 13:26:58.8 | −62:03:25 | 71 | 8 | A | C8, DC, E8, S |
| 12 | 309.421 | −0.621 | 13:48:38.1 | −62:46:11 | 48 | 10 | A | DC |
| 13 | 309.537 | −0.742 | 13:49:51.6 | −62:51:42 | 38 | 7 | A | C8, DC, E8 |
| 14 | 309.968 | 0.302 | 13:51:25.6 | −61:44:51 | 40 | 6 | A | DC, E8 |
| 15 | 309.996 | 0.507 | 13:51:15.8 | −61:32:30 | 88 | 8 | A | E8, DC |
| 16 | 313.762 | −0.860 | 14:24:58.6 | −61:44:56 | 80 | 15 | A | BR,C8, DC, E4, E8, U8 |
| 17 | 314.203 | 0.213 | 14:25:15.4 | −60:35:22 | 86 | 12 | A | C8, E8, U8 |
| 18 | 314.269 | 0.092 | 14:26:06.6 | −60:40:43 | 87 | 8 | A | C8, DC, E8, S, V2 |
| 19 | 317.466 | −0.401 | 14:51:19.3 | −59:50:46 | 45 | 7 | A | DC, E4, E8 |
| 20 | 317.884 | −0.253 | 14:53:45.6 | −59:31:34 | 74 | 15 | A | DC, E4, E8 |
| 21 | 318.049 | 0.088 | 14:53:42.2 | −59:08:49 | 88 | 20 | A | C8, DC, U8 |
| 22 | 318.777 | −0.144 | 14:59:33.5 | −59:00:59 | 105 | 8 | A | B, E8, V2 |
| 23 | 319.336 | 0.912 | 14:59:31.0 | −57:49:18 | 65 | 12 | A | |
| 24a | 321.937 | −0.006 | 15:19:43.2 | −57:18:04 | 33 | 9 | A | C8, DC, E8 |
| 25 | 321.952 | 0.014 | 15:19:44.6 | −57:16:35 | 37 | 10 | A | E8 |
| 26 | 326.476 | 0.699 | 15:43:18.0 | −54:07:23 | 81 | 12 | A | C8, DC, E4, U8 |
| 27 | 326.796 | 0.385 | 15:46:20.3 | −54:10:35 | 54 | 10 | A | DC, E4 |
| 28 | 328.165 | 0.587 | 15:52:42.6 | −53:09:48 | 31 | 6 | A | E4, U8 |
| 29a | 328.252 | −0.531 | 15:57:58.9 | −53:58:02 | 58 | 9 | A | C8, DC, E4, E8 |
| 30 | 328.809 | 0.635 | 15:55:48.4 | −52:43:00 | 82 | 9 | V | C8, DC, E4 |
| 31 | 329.184 | −0.313 | 16:01:47.0 | −53:11:40 | 73 | 8 | A | DC, E4, U8 |
| 32a | 330.031 | 1.043 | 16:00:09.4 | −51:36:52 | 56 | 6 | A | DC, E8, S |
| 33 | 335.061 | −0.428 | 16:29:23.5 | −49:12:25 | 63 | 6 | A | C8, DC, E4 |
| 34 | 337.153 | −0.393 | 16:37:48.5 | −47:38:53 | 49 | 4 | A | DC, U8, V2 |
| 35 | 338.396 | −0.406 | 16:42:43.2 | −46:43:36 | 65 | 8 | A | C8, DC, E4 |
| 36 | 338.922 | 0.390 | 16:41:15.7 | −45:48:23 | 97 | 11 | A | C8, E8, S |
| 37 | 338.930 | −0.495 | 16:45:08.6 | −46:22:50 | 80 | 11 | A | C8, DC, E8, U8 |
| 38 | 339.584 | −0.127 | 16:45:59.1 | −45:38:44 | 53 | 9 | A | DC, E4, E8 |
| 39a | 344.221 | −0.569 | 17:04:06.6 | −42:18:57 | 51 | 11 | A | BR, E4, E8 |
| 40 | 344.996 | −0.224 | 17:05:09.7 | −41:29:26 | 75 | 15 | A | DC, E4, U8 |
| 41 | 347.883 | −0.291 | 17:14:27.3 | −39:12:35 | 62 | 6 | V | C8, E8 |
| 42 | 348.180 | 0.483 | 17:12:08.1 | −38:30:54 | 38 | 7 | A | E8 |
| 43 | 348.584 | −0.920 | 17:19:11.6 | −39:00:08 | 52 | 10 | A | C8, E4 |
| 44 | 350.105 | 0.085 | 17:19:26.7 | −37:10:48 | 167 | 25 | A | C8, E8, V2 |
| 45 | 350.930 | 0.753 | 17:19:04.7 | −36:07:16 | 90 | 14 | A | C8, DC, E8, S |
| 46 | 351.776 | −0.538 | 17:26:43.1 | −36:09:18 | 93 | 14 | A | C8, DC, E4, E8 |
| 47 | 352.489 | 0.797 | 17:23:15.6 | −34:48:53 | 84 | 7 | A | C8, E8 |
| 48 | 358.386 | −0.482 | 17:43:37.5 | −30:33:51 | 57 | 5 | A | C8, DC, E4, E8, V2 |
| 49 | 0.675 | −0.046 | 17:47:23.7 | −28:22:59 | 140 | 23 | A | C8, E8, S |
| 50 | 4.001 | 0.335 | 17:53:34.5 | −25:19:57 | 56 | 12 | A | BR, C8, E8 |
| 51 | 5.636 | 0.239 | 17:57:33.9 | −23:58:05 | 65 | 7 | A | C8, DC, E8 |
| 52 | 6.797 | −0.256 | 18:01:57.6 | −23:12:26 | 50 | 11 | A | C8, DC, E4, U8 |
| 53 | 8.492 | −0.633 | 18:06:59.3 | −21:54:55 | 126 | 28 | A | DC, S |
| 54 | 9.221 | 0.166 | 18:05:31.3 | −20:53:21 | 42 | 7 | A | DC, E8 |
| 55 | 14.113 | −0.571 | 18:18:12.4 | −16:57:18 | 57 | 9 | A | DC, E8 |
| 56 | 14.341 | −0.642 | 18:18:55.2 | −16:47:15 | 124 | 15 | A | C8, DC, E4, E8 |
| 57 | 17.168 | 0.815 | 18:19:08.4 | −13:36:29 | 61 | 12 | A | DC |
| 58 | 25.297 | 0.309 | 18:36:20.5 | −06:38:57 | 39 | 8 | A | E8 |
| 59 | 26.507 | 0.284 | 18:38:40.0 | −05:35:06 | 49 | 7 | A | C8, DC |
| 60 | 31.158 | 0.047 | 18:48:02.1 | −01:33:26 | 50 | 8 | A | E8 |
| 61 | 34.403 | 0.229 | 18:53:18.4 | 01:24:47 | 91 | 8 | A | DC, E4 |
| 62 | 39.497 | −0.993 | 19:07:00.0 | 05:23:05 | 53 | 7 | A | C8, V2 |
| 63 | 43.040 | −0.451 | 19:11:38.7 | 08:46:40 | 52 | 6 | A | C8, E4, E8 |
| 64 | 43.893 | −0.785 | 19:14:26.8 | 09:22:44 | 63 | 7 | A | C8, E8 |
| 65 | 47.874 | 0.309 | 19:18:04.1 | 13:24:41 | 68 | 11 | A | C8, E8 |
| 66 | 49.912 | 0.369 | 19:21:47.7 | 15:14:20 | 55 | 11 | V | BR, C8, E8 |
| 67 | 50.053 | 0.064 | 19:23:11.3 | 15:13:10 | 107 | 14 | A | DC, S |
| 68 | 52.570 | −0.955 | 19:31:54.7 | 16:56:44 | 44 | 9 | A | E4, E8 |
| 69 | 53.147 | 0.071 | 19:29:18.0 | 17:56:41 | 119 | 13 | A | C8, DC, S |
| 70 | 53.237 | 0.056 | 19:29:32.3 | 18:00:57 | 76 | 19 | A | DC, S |
| 71 | 56.961 | −0.234 | 19:38:16.7 | 21:08:02 | 58 | 8 | A | C8, E8 |
| 72 | 58.471 | 0.432 | 19:38:58.4 | 22:46:32 | 73 | 10 | A | C8, E8 |
| 73 | 59.783 | 0.071 | 19:43:09.9 | 23:44:14 | 120 | 11 | A | C8, E4, E8, V2 |
| 74 | 62.379 | 0.298 | 19:48:02.4 | 26:05:51 | 47 | 7 | A | |
| 75 | 64.272 | −0.425 | 19:55:09.4 | 27:21:18 | 55 | 10 | A | BR |
Notes. Units of right ascension are hours, minutes, and seconds, and units of declination are degrees, arcminutes, and arcseconds. Column 6 gives the estimated angular diameter. Column 7 gives the estimated number of stellar members within the assumed radius, considered as a lower limit due to possible non-detection of low-mass stars. Column 8 indicates the detection method: automated search (A), or on-line viewer (V). Column 9 lists different flags determined after visual inspection of the GLIMPSE three-color images, indicating: association with extended 8.0 μm emission (E8) or localized diffuse 4.5 μm emission (E4); cluster embedded in an infrared dark cloud (DC); cluster composed of red sources and additional bright normal stars (BR); cluster composed of bright normal stars alone (B); presence of additional probable YSOs, identified as sources uniquely detected at 8.0 μm (U8), or compact 8.0 μm objects not listed in the point source catalog or archive (C8); sparse, not centrally condensed morphology (S); cluster identified by-eye in a nearby location of an automatically detected overdensity, but not exactly at the same position (V2).
Contained within a cluster from the Majaess (2013) catalog: clusters with IDs 147, 161, 167, 169, and 177 contain clusters G3CC 4, 24, 29, 32, and 39, respectively.
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