Table 7
A list of potential ALMA candidates.
| RRL peak flux | Radio continuum source | |||||||
|---|---|---|---|---|---|---|---|---|
| ATLASGAL | RA | Dec | Dist. | mm | submm | Size | Peak flux | Morphology |
| name | α(J2000) | δ(J2000) | (kpc) | (Jy) | (Jy) | (″) | (mJy/beam) | |
| AGAL010.624−00.384 | 18:10:28.70 | −19:55:49.1 | 5.0 | 6.6 | 10.0 | 4.6 | 305.6 | Core-halo |
| AGAL012.804−00.199 | 18:14:13.96 | −17:55:44.9 | 2.6 | 10.2 | 17.5 | 16.2 | 287.9 | Bipolar? |
| AGAL013.872+00.281 | 18:14:35.81 | −16:45:37.2 | 3.9 | 2.2 | 4.8 | 15.4 | 24.7 | Cometary |
| AGAL032.797+00.191 | 18:50:30.95 | −00:01:56.5 | 13.0 | 2.8 | 6.9 | 10.0 | 279.1 | Cometary or multi-peaks |
| AGAL037.874−00.399 | 19:01:53.59 | +04:12:51.7 | 9.7 | 2.0 | 4.1 | 8.9 | 255.7 | Cometary? |
| AGAL043.164−00.029 | 19:10:22.01 | +09:05:03.2 | 11.3 | 2.3 | 4.6 | 9.6 | 242.9 | Cometary |
| AGAL045.121+00.131 | 19:13:27.96 | +10:53:35.7 | 8.0 | 3.2 | 6.9 | 7.5 | 299.7 | Cometary? or bipolar? |
| AGAL045.454+00.061 | 19:14:21.31 | +11:09:11.7 | 8.4 | 1.4 | 3.7 | 7.6 | 61.8 | Unresolved |
| AGAL298.224−00.339 | 12:10:01.18 | −62:49:54.0 | 11.4 | ... | 6.6 | 4.1 | 369.9 | Cometary |
| AGAL298.859−00.437 | 12:15:25.27 | −63:01:17.0 | 10.1 | ... | 4.0 | 2.6 | 79.5 | Unresolved |
| AGAL324.201+00.121 | 15:32:53.21 | −55:56:11.8 | 6.8 | 2.2 | 4.1 | 6.1 | 286.6 | Cometary (& unresolved) |
| AGAL330.954−00.182 | 16:09:52.54 | −51:54:54.9 | 5.3 | 4.1 | 8.7 | 3.9 | 444.4 | Unresolved |
| AGAL332.156−00.449 | 16:16:40.53 | −51:17:08.9 | 3.6 | 2.4 | 6.7 | 14.0 | 101.2 | Irregular |
| AGAL332.826−00.549 | 16:20:11.10 | −50:53:15.4 | 3.6 | 4.9 | 10.9 | 3.4 | 461.6 | Unresolved(bipolar?) |
| AGAL333.284−00.387 | 16:21:31.70 | −50:27:00.5 | 3.6 | 7.8 | 11.4 | 9.4 | 421.4 | Irregular (cometary?) |
| AGAL333.604−00.212 | 16:22:09.58 | −50:05:59.6 | 3.6 | 40.8 | 47.5 | 10.6 | 393.6 | Irregular |
| AGAL345.649+00.009 | 17:06:15.99 | −40:49:45.4 | 1.4 | 2.1 | 2.5 | 5.1 | 627.4 | Core-halo |
Notes. The coordinates provided here are coordinates of radio continuum sources in the ATLASGAL clumps instead of coordinates of the ATLASGAL clumps. Ambiguous morphology of the radio continuum emission is indicated with a question mark, “?”.
References. Distance: Urquhart et al. (2013a), Lumsden et al. (2013), Urquhart et al. (2018). Coordinate & radio continuum source: Purcell et al. (2013), Urquhart et al. (2007).
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