Table 2
Physical properties of fragments in Musca.
# | RA | Dec |
![]() |
F 870,peak | R | M NIR | ⟨ n ⟩ | Region |
[1021 cm-2] | [Jy beam-1] | [pc] | [M⊙] | [104 cm-3] | ||||
|
||||||||
1 | 12:21:26 | –72:21:06 | 23 | 0.15 | 0.07 | 2.5 | 4 | South |
2 | 12:21:54 | –72:17:02 | 19 | 0.11 | 0.07 | 1.7 | 3 | South |
3a | 12:22:19 | -72:10:24 | 17 | 0.10 | 0.06 | 1.0 | 2 | South |
4 | 12:24:32 | –71:50:23 | 27 | 0.22 | 0.08 | 3.5 | 3 | South |
5 | 12:25:37 | –71:42:14 | 34 | 0.18 | 0.11 | 7.1 | 3 | South |
|
||||||||
6 | 12:26:46 | –71:30:00 | 15 | 0.10 | 0.07 | 1.7 | 3 | Center |
7 | 12:26:59 | –71:27:41 | 17 | 0.10 | 0.06 | 1.2 | 3 | Center |
8b | 12:27:45 | –71:22:07 | 15 | 0.10 | 0.05 | 1.3 | 3 | Center |
9c | 12:29:46 | –71:22:42 | 6 | 0.05 | 0.04 | 0.5 | 1 | Center |
10a | 12:28:30 | –71:18:13 | 17 | 0.12 | 0.04 | 1.4 | 4 | Center |
11a | 12:29:26 | –71:10:41 | 20 | 0.17 | 0.05 | 1.4 | 3 | Center |
|
||||||||
12 | 12:30:48 | –71:10:08 | 15 | 0.14 | 0.05 | 0.9 | 4 | North |
13 | 12:31:03 | –71:04:32 | 19 | 0.10 | 0.04 | 1.1 | 6 | North |
14 | 12:31:05 | –71:01:54 | 19 | 0.09 | 0.04 | 0.9 | 5 | North |
15 | 12:31:53 | –71:02:08 | 17 | 0.07 | 0.07 | 1.8 | 3 | North |
16 | 12:32:13 | –70:57:49 | 13 | 0.06 | 0.04 | 0.6 | 4 | North |
17 | 12:34:09 | –70:57:40 | 7 | 0.06 | 0.04 | 0.3 | 2 | North |
18 | 12:34:24 | –70:56:11 | 8 | 0.08 | 0.04 | 0.3 | 2 | North |
19 | 12:32:41 | –70:44:21 | 15 | 0.19 | 0.06 | 1.0 | 2 | North |
20 | 12:35:00 | –70:43:54 | 11 | 0.12 | 0.05 | 0.6 | 3 | North |
21 | 12:35:17 | –70:40:10 | 30 | 0.62 | 0.05 | 1.1 | 5 | North |
Notes.
The peak value of dust emission from the fragment is more than 45′′ offset from the associated extinction peak. The structure is considered a fragment because the contours outlining the local maximum in emission overlap with the contours outlining a local maximum in extinction. The mass estimate is based on extinction data; the aperture for the mass calculation was centered on the nearest extinction maximum.
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