Table A.1
Properties of the observed sources: results from a 2D Gaussian fit, bolometric temperatures, and bolometric luminosities.
Source | Common names | R. A. (J2000) (hh:mm:ss) | Dec (J2000) (dd:mm:ss) | F1.2 mm (mJy beam−1) | Tbol (K)(a) | Lbol (L⊙)(a) |
---|---|---|---|---|---|---|
Class 0 (Tbol ≤ 70 K) | ||||||
Per-emb 1 | HH 211 MMS | 03:43:56.81 | +32:00:50.2 | 42.9 ± 2.7 | 27 ± 1 | 1.80 ± 0.10 |
Per-emb 2 | IRAS 03292+3039 | 03:32:17.92 | +30:49:47.8 | 66.3 ± 2.8 | 27 ± 1 | 0.90 ± 0.07 |
Per-emb 5 | IRAS 03282+3035 | 03:31:20.94 | +30:45:30.2 | 138.7 ± 1.7 | 32 ± 2 | 1.30 ± 0.10 |
Per-emb 8 | 03:44:43.98 | +32:01:35.2 | 79.9 ± 1.7 | 43 ± 6 | 2.60 ± 0.50 | |
Per-emb 10 | B1-d | 03:33:16.43 | +31:06:52.0 | 18.5 ± 0.2 | 30 ± 2 | 0.60 ± 0.05 |
Per-emb 11 A(b) | IC 348 MMS | 03:43:57.07 | +32:03:04.8 | 97.3 ± 2.7 | 34 ± 36 | 1.12 ± 0.34 |
Per-emb 11 B(b) | IC 348 MMS | 03:43:56.88 | +32:03:03.0 | 4.2 ± 0.4 | 34 ± 36 | 1.12 ± 0.34 |
Per-emb 11 C | IC 348 MMS | 03:43:57.70 | +32:03:09.9 | 4.0 ± 0.4 | 36 ± 65 | 0.10 ± 0.03 |
Per-emb 12 A(b) | NGC 1333 IRAS4 A2 | 03:29:10.54 | +31:13:30.9 | 411 ± 39 (e) | 29 ± 2 | 3.50 ± 0.70 |
Per-emb 12 B(b) | NGC 1333 IRAS4 A1 | 03:29:10.44 | +31:13:32.1 | 209 ± 17 | 29 ± 2 | 3.50 ± 0.70 |
Per-emb 13 | NGC 1333 IRAS4 B1 | 03:29:12.02 | +31:13:08.0 | 303.8 ± 8.8 | 28 ± 1 | 4.00 ± 0.30 |
Per-emb 14 | NGC 1333 IRAS4 C | 03:29:13.55 | +31:13:58.1 | 66.4 ± 0.7 | 31 ± 2 | 0.70 ± 0.08 |
Per-emb 15 | 03:29:04.06 | +31:14:46.2 | 3.2 ± 0.3 | 36 ± 4 | 0.40 ± 0.10 | |
Per-emb 16 | 03:43:50.98 | +32:03:24.1 | 3.3 ± 0.3 | 39 ± 2 | 0.40 ± 0.04 | |
Per-emb 17 | L1455 IRS1 | 03:27:39.11 | +30:13:03.0 | 32.9 ± 0.9 | 59 ± 11 | 4.20 ± 0.10 |
Per-emb 18 | NGC 1333 IRAS7 SM1 | 03:29:11.27 | +31:18:31.1 | 70.2 ± 1.1 | 46 ± 12 | 4.70 ± 0.72 |
Per-emb 20 | L1455 IRS4 | 03:27:43.28 | +30:12:28.9 | 2.6 ± 0.2 | 65 ± 3 | 1.40 ± 0.20 |
Per-emb 21 | NGC 1333 IRAS7 SM2 | 03:29:10.67 | +31:18:20.2 | 44.2 ± 1.1 | 52 ± 17 | 3.42 ± 0.53 |
Per-emb 22 A(b) | L1448 IRS2 | 03:25:22.41 | +30:45:13.3 | 30.3 ± 1.3 | 51 ± 12 | 2.15 ± 0.66 |
Per-emb 22 B(b) | L1448 IRS2 | 03:25:22.37 | +30:45:13.2 | 17.1 ± 0.1 | 51 ± 12 | 2.15 ± 0.66 |
Per-emb 25 | IRAS 03235+3004 | 03:26:37.51 | +30:15:27.8 | 89.9 ± 0.2 | 61 ± 12 | 1.20 ± 0.02 |
Per-emb 26 | L1448-mm | 03:25:38.88 | +30:44:05.3 | 137.5 ± 2.7 | 47 ± 7 | 8.40 ± 1.50 |
Per-emb 27 | NGC 1333 IRAS 2A | 03:28:55.57 | +31:14:37.0 | 118.1 ± 8.2 | 49 ± 10 | 47.06 ± 7.21 |
Per-emb 28 | 03:43:51.01 | +32:03:08.0 | 13.8 ± 0.4 | 45 ± 2 | 0.70 ± 0.08 | |
Per-emb 29 | B1-c | 03:33:17.88 | +31:09:31.7 | 73.4 ± 3.6 | 48 ± 1 | 3.70 ± 0.40 |
Per-emb 33 A(b) | L1448 IRS 3B | 03:25:36.38 | +30:45:14.8 | 156.0 ± 8.8 | 57 ± 3 | 2.77 ± 0.80 |
Per-emb 33 B/C(b) | L1448 IRS 3B | 03:25:36.32 | +30:45:15.0 | 84.3 ± 1.2 | 57 ± 3 | 5.53 ± 0.80 |
Per-emb 36 | NGC 1333 IRAS 2B | 03:28:57.38 | +31:14:15.8 | 118.9 ± 0.6 | 48 ± 1 | 5.27 ± 0.81 |
Per-emb 37 | 03:29:18.97 | +31:23:14.3 | 11.6 ± 0.6 | 22 ± 1 | 0.50 ± 0.10 | |
IRAS 4B2 | NGC 1333 IRAS4 B2 | 03:29:12.84 | +31:13:06.9 | 146.2 ± 3.9 | 9±1 | 1.76 ± 0.28 |
B1-bN | 03:33:21.21 | +31:07:43.6 | 69.3 ± 1.7 | 22 ± 1 | 0.16 ± 0.02 | |
B1-bS | 03:33:21.36 | +31:07:26.3 | 134.1 ± 1.4 | 24 ± 11 | 0.32 ± 0.05 | |
L1448 IRS 2E(c) | 03:25:25.66 | +30:44:56.7 | – | 15 | 0.05 ± 0.05 | |
L1448 NW | L1448 IRS 3C | 03:25:35.67 | +30:45:34.2 | 55.2 ± 1.8 | 43 ± 1 | 2.89 ± 0.44 |
L1448 IRS 3A | 03:25:36.50 | +30:45:21.9 | 52.5 ± 2.5 | 57 ± 10 | 8.08 ± 1.27 | |
SVS 13 B | 03:29:03.08 | +31:15:51.7 | 135.5 ± 5.2 | 36 ± 1 | 10.26 ± 1.57 | |
Class I (Tbol ≥ 70 K) | ||||||
Per-emb 35 A(b) | NGC 1333 IRAS1 | 03:28:37.10 | +31:13:30.8 | 20.6 ± 0.6 | 103 ± 26 | 4.55 ± 0.30 |
Per-emb 35 B(b) | NGC 1333 IRAS1 | 03:28:37.22 | +31:13:31.7 | 16.1 ± 0.7 | 103 ± 26 | 4.55 ± 0.30 |
Per-emb 40 | B1-a | 03:33:16.67 | +31:07:54.9 | 13.7 ± 0.2 | 132 ± 25 | 1.50 ± 1.00 |
Per-emb 41(d) | B1-bW | 03:33:20.34 | +31:07:21.3 | 11.4 ± 0.5 | 157 ± 72 | 0.17 ± 0.36 |
Per-emb 42 | L1448C-S | 03:25:39.14 | +30:43:57.9 | 11.1 ± 0.3 | 83 ± 12 | 1.98 ± 0.31 |
Per-emb 44 | NGC 1333 SVS 13A | 03:29:03.76 | +31:16:03.7 | 132.0 ± 7.4 | 75 ± 52 | 119.28 ± 18.31 |
Per-emb 50 | IRAS 03260+3111 A | 03:29:07.77 | +31:21:57.1 | 87.4 ± 0.3 | 128 ± 23 | 23.20 ± 3.00 |
Per-emb 53 | B5 IRS1 | 03:47:41.59 | +32:51:43.6 | 14.8 ± 0.2 | 287 ± 8 | 4.70 ± 0.90 |
Per-emb 54 | NGC 1333 IRAS6 | 03:29:01.55 | +31:20:20.5 | 1.5 ± 0.1 | 131 ± 63 | 16.80 ± 2.60 |
Per-emb 55 | IRAS 03415+3152 | 03:44:43.30 | +32:01:31.2 | 3.4 ± 0.1 | 334 ± 340 | 1.49 ± 0.25 |
Per-emb 60 | 03:29:20.05 | +31:24:07.4 | 1.6 ± 0.1 | 363 ± 240 | 0.28 ± 1.05 | |
L1455 IRS 2 | 03:27:47.69 | +30:12:04.4 | 2.1 ± 0.1 | 740 | 2.50 ± 0.10 | |
EDJ2009-172 | 03:28:56.65 | +31:18:35.4 | 13.6 ± 0.1 | 1100 | 0.39 ± 0.10 | |
EDJ2009-235 | 03:29:18.26 | +31:23:19.7 | 5.5 ± 0.1 | 291 ± 14 | 0.02 ± 0.02 | |
Unknown Tbol | ||||||
SVS 13 A2 | VLA3 | 03:29:03.39 | +31:16:01.6 | 13.9 ± 0.8 | – | – |
EDJ2009-237 | 03:29:18.74 | +31:23:25.2 | 2.5 ± 0.2 | – | 0.02 | |
RAC1999 VLA20 | 03:29:04.25 | +31:16:09.1 | 5.8 ± 0.2 | – | – |
Notes. (a)From Tobin et al. (2016) and Murillo et al. (2016). (b)Lbol values divided by the amount of components (unresolved binaries and triple systems). (c)No continuum detection. (d)Edge of the field of view. (e)Optically thick continuum emission.
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