Table 3
Parameters of the 15 cores detected in the LABOCA map with Clumpfind (see Fig. 1).
# | Ra | Dec | FWHMx | FWHM y | Imax | Ftot | Mcore | Tcore | Counterpart |
[″] | [″] | [Jy/beam] | [Jy] | [M⊙] | [K] | ||||
|
|||||||||
1 | 15:43:01.68 | −34:09:08.9 | 58.22 | 44.38 | 1.37 | 5.61 | 1.71 | 14.0 | Lup1 C4 |
2 | 15:44:59.85 | −34:17:08.8 | 62.51 | 44.09 | 0.51 | 3.97 | 1.59 | 12.0 | Lup1 C6 |
3 | 15:45:13.58 | −34:17:08.8 | 46.56 | 33.45 | 0.33 | 1.48 | 0.40 | 15.0 | Lup1 C7 |
4 | 15:45:16.02 | −34:16:56.6 | 35.31 | 34.95 | 0.31 | 1.00 | 0.27 | 15.0 | Lup1 C7 |
5 | 15:45:03.80 | −34:17:57.3 | 57.22 | 42.24 | 0.28 | 1.41 | 0.46 | 13.5 | Lup1 C6 |
6 | 15:42:52.86 | −34:08:02.1 | 96.42 | 49.94 | 0.28 | 3.85 | 1.34 | 13.0 | Lup1 C3 |
7 | 15:42:43.57 | −34:08:14.2 | 70.62 | 44.38 | 0.25 | 1.64 | 0.57 | 13.0 | Lup1 C3 |
8 | 15:42:44.55 | −34:08:32.5 | 30.55 | 20.85 | 0.25 | 0.48 | 0.17 | 13.0 | Lup1 C3 |
9 | 15:42:44.06 | −34:08:44.6 | 36.82 | 19.26 | 0.24 | 0.49 | 0.17 | 13.0 | Lup1 C3 |
10 | 15:42:50.42 | −34:08:38.5 | 53.28 | 30.34 | 0.22 | 1.05 | 0.36 | 13.0 | Lup1 C3 |
11 | 15:45:25.10 | −34:24:01.8 | 42.46 | 69.57 | 0.22 | 1.63 | 0.53 | 13.5 | Lup1 C8 |
12 | 15:42:23.02 | −34:09:33.2 | 68.97 | 46.08 | 0.21 | 1.72 | 0.53 | 14.0 | Lup1 C1 |
13 | 15:39:09.92 | −33:25:30.9 | 27.24 | 27.70 | 0.20 | 0.34 | 0.07 | 17.0 | – |
14 | 15:45:55.75 | −34:29:23.7 | 28.10 | 26.28 | 0.20 | 0.29 | 0.08 | 14.5 | – |
15 | 15:42:47.90 | −33:53:15.3 | 43.80 | 19.59 | 0.19 | 0.43 | 0.12 | 15.0 | Lup1 C2 |
Notes. The beam size (HPBW) and area used to convert intensities into fluxes is 21.2″ and 509 arcsec2, respectively. The total mass of all cores is ≈8 M⊙. Columns 4 and 5 give the FWHM of the ellipses representing the cores. Columns 6−8 give the core’s peak intensity, total flux, and mass, respectively. The core temperature shown in Col. 9 was derived from the Herschel SPIRE SED fit temperature map as a mean temperature within the ellipse representing the core. The last column gives the matches to dense cores found by Benedettini et al. (2012).
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