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Table D.1
General source information of the 24 protostars in our sample.
| Source | Other Names | Subregion | RA (J2000) | DEC (J2000) | Class | Lbol(a) | Tbol(a) | Tkin(b) | Hot |
|---|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss) | (dd:mm:ss) | (L⊙) | (K) | (K) | Corino | ||||
| BlbN | Barnard 1 | 03:33:21.21 | 31:07:43.6 | 0 | 0.32±0.10 | 14.7±1.0 | 100.0 | Ν | |
| BlbS | Barnard 1 | 03:33:21.36 | 03:07:26.3 | 0 | 0.70±0.01 | 17.7±1.0 | 100.0 | Y | |
| B5-IRS1 | Per-emb-53 | Barnard 5 | 03:47:41.59 | 32:51:43.6 | I | 4.70±0.90 | 287.0±8.0 | 287.0 | Ν |
| HH211MMS | Per-emb-01 | IC348 | 03:43:56.81 | 32:00:50 | 0 | 1.80±0.10 | 27.0±1.0 | 100.0 | Y |
| IC348MMS | Per-emb-11 | IC348 | 03:43:57.07 | 32:03:04.8 | 0 | 1.50±0.10 | 30.0±2.0 | 100.0 | Y |
| IRAS2A | Per-emb-27 | NGC1333 | 03:28:55.57 | 31:14:37.0 | 0/I | 19.00±0.40 | 69.0±1.0 | 100.0 | Y |
| IRAS2B | Per-emb-36 | NGC1333 | 03:28:57.38 | 31:14:15.8 | I | 5.30±1.00 | 106.0±12.0 | 106.0 | Ν |
| IRAS4B | Per-emb-13 | NGC1333 | 03:29:12.02 | 31:13:08.0 | 0 | 4.00±0.30 | 28.0±1.0 | 100.0 | Y |
| IRAS4C | Per-emb-14 | NGC1333 | 03:29:13.55 | 31:13:58.1 | 0 | 0.70±0.08 | 31.0±2.0 | 100.0 | Ν |
| L1448-IRS3A | L1448 | 03:25:36:50 | 30:45:21.9 | 0 | 9.20±1.30 | 47.0±2.0 | 100.0 | Ν | |
| L1448-IRS3B | Per-emb-33 | L1448 | 03:25:36.38 | 30:45:14.7 | 0 | 8.30±0.80 | 57.0±3.0 | 100.0 | Ν |
| L1448C | Per-emb-26 | L1448 | 03:25:38.88 | 30:44:05.3 | 0 | 8.40±1.50 | 47.0±7.0 | 100.0 | Y |
| L1448NW | L1448-IRS3C | L1448 | 03:25:35.67 | 30:45:34.2 | 0 | 1.40±0.10 | 22.0±1.0 | 100.0 | Ν |
| Per-emb-02 | Barnard 1 | 03:32:17.92 | 30:49:47.8 | 0 | 0.90±0.07 | 27.0±1.0 | 100.0 | Ν | |
| Per-emb-05 | … (c) | 03:31:20.94 | 30:45:30.2 | 0 | 1.30±0.10 | 32.0±2.0 | 100.0 | Ν | |
| Per-emb-08 | IC348 | 03:44:43.98 | 32:01:35.2 | 0 | 2.60±0.50 | 43.0±6.0 | 100.0 | Ν | |
| Per-emb-18 | IRAS7 | NGC1333 | 03:29:11.27 | 31:18:31.1 | 0 | 2.80±1.70 | 59.0±12.0 | 100.0 | Ν |
| Per-emb-22 | L1448-IRS2 | L1448 | 03:25:22.41 | 30:45:13.3 | 0 | 3.60±0.50 | 43.0±2.0 | 100.0 | Ν |
| Per-emb-29 | Blc | Barnard 1 | 03:33:17.88 | 31:09:31.7 | 0 | 3.70±0.40 | 48.0±1.0 | 100.0 | Ν |
| Per-emb-30 | Barnard 1 | 03:33:27.28 | 31:07:10.2 | 0/I | 1.70±0.01 | 78.0±6.0 | 100.0 | Ν | |
| Per-emb-50 | NCG1333 | 03:29:07.77 | 31:21:57.1 | I | 23.20±3.00 | 128.0±23.0 | 128.0 | Ν | |
| Per-emb-62 | IC348 | 03:44:12.98 | 32:01:35.4 | I | 1.80±0.40 | 378.0±29.0 | 378.0 | Ν | |
| SVS13A | Per-emb-44 | NGC1333 | 03:29:03.76 | 31:16:03.7 | 0/I | 32.50±7.10 | 188.0±9.0 | 188.0 | Υ |
| SVS13B | NGC1333 | 03:29:03.08 | 31:15:51.7 | 0 | 1.00±1.00 | 20.0±20.0 | 100.0 | Ν |
Notes. (a) Data extracted from Tobin et al. (2016b). (b) We have assumed the Tkin of the warm inner core to be the maximum between 100K and Tkin (which implies, Τ ≥ 100K).(c) Close to the Barnard 1 region, but isolated.
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