Table 1
LABOCA 870 μm clumps in G304.74.
| Source | α 2000.0 | δ 2000.0 | S/N |
|
S 870 | R eff | |
| [h:m:s] | [°:′:″] | [Jy beam-1] | [Jy] | [′′] | [pc] | ||
|
|
|||||||
| SMM 1 | 13 06 20.89 | –61 30 20.51 | 12.1 | 0.48 ± 0.07 | 1.53 ± 0.18 | 25.1 | 0.31 ± 0.08 |
| SMM 2 | 13 06 29.29 | –61 29 36.67 | 9.1 | 0.36 ± 0.05 | 0.63 ± 0.06 | 17.0 | 0.21 ± 0.05 |
| SMM 3 | 13 06 36.56 | –61 28 52.79 | 11.1 | 0.44 ± 0.07 | 0.82 ± 0.11 | 15.8 | 0.19 ± 0.05 |
| SMM 4 | 13 06 46.06 | –61 28 40.90 | 14.6 | 0.58 ± 0.08 | 1.47 ± 0.17 | 18.5 | 0.23 ± 0.06 |
| IRAS 13037-6112 | 13 06 51.65 | –61 27 56.95 | 11.5 | 0.46 ± 0.07 | 1.24 ± 0.14 | 14.5 | 0.18 ± 0.05 |
| SMM 5 | 13 06 50.54 | –61 27 08.94 | 6.2 | 0.25 ± 0.05 | 0.28 ± 0.05 | 11.7 | 0.14 ± 0.04 |
| SMM 6 | 13 06 53.88 | –61 27 32.96 | 10.3 | 0.41 ± 0.06 | 0.41 ± 0.06 | < 9.9 | < 0.15 |
| SMM 7 | 13 07 03.38 | –61 26 17.00 | 8.1 | 0.33 ± 0.05 | 0.52 ± 0.07 | 14.0 | 0.17 ± 0.04 |
| IRAS 13039-6108 | 13 07 07.28 | –61 24 33.00 | 12.8 | 0.51 ± 0.07 | 1.41 ± 0.16 | 17.4 | 0.21 ± 0.06 |
| SMM 8 | 13 07 09.51 | –61 23 41.00 | 7.0 | 0.28 ± 0.05 | 0.28 ± 0.05 | < 9.9 | < 0.15 |
| SMM 9 | 13 07 12.85 | –61 22 44.99 | 11.2 | 0.45 ± 0.07 | 0.83 ± 0.10 | 13.0 | 0.16 ± 0.04 |
| IRAS 13042-6105 | 13 07 21.74 | –61 21 40.95 | 5.8 | 0.23 ± 0.05 | 0.23 ± 0.05 | < 9.9 | < 0.15 |
|
|
|||||||
| BLOB 1a | 13 06 40.46 | –61 29 20.84 | 8.2 | 0.33 ± 0.05 | 0.33 ± 0.05 | < 9.9 | < 0.15 |
| BLOB 2a | 13 06 40.44 | –61 29 52.84 | 6.8 | 0.27 ± 0.05 | 0.31 ± 0.05 | 10.2 | 0.13 ± 0.03 |
Notes. The columns are as follows: (1) source name; (2) and (3): coordinates of the emission peak position; (4) S/N of the source; (5) peak intensity; (6) integrated flux density; (7) and (8) effective radius of the clump in angular and linear units. The clumps SMM 6, SMM 8, IRAS 13042, and BLOB 1 have an effective radius smaller than half the beam FWHM, and are hence considered as unresolved sources.
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