Open Access

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 31:07:43.60 0.32±0.10 14.7±1.0 100.0 Ν
BlbS Barnard 1 03:33:21.36 03:07:26.30 0.70±0.01 17.7±1.0 100.0 Y
B5-IRS1 Per-emb-53 Barnard 5 03:47:41.59 32:51:43.6I 4.70±0.90 287.0±8.0 287.0 Ν
HH211MMS Per-emb-01 IC348 03:43:56.81 32:00:500 1.80±0.10 27.0±1.0 100.0 Y
IC348MMS Per-emb-11 IC348 03:43:57.07 32:03:04.80 1.50±0.10 30.0±2.0 100.0 Y
IRAS2A Per-emb-27 NGC1333 03:28:55.57 31:14:37.00/I 19.00±0.40 69.0±1.0 100.0 Y
IRAS2B Per-emb-36 NGC1333 03:28:57.38 31:14:15.8I 5.30±1.00 106.0±12.0 106.0 Ν
IRAS4B Per-emb-13 NGC1333 03:29:12.02 31:13:08.00 4.00±0.30 28.0±1.0 100.0 Y
IRAS4C Per-emb-14 NGC1333 03:29:13.55 31:13:58.10 0.70±0.08 31.0±2.0 100.0 Ν
L1448-IRS3A L1448 03:25:36:50 30:45:21.90 9.20±1.30 47.0±2.0 100.0 Ν
L1448-IRS3B Per-emb-33 L1448 03:25:36.38 30:45:14.70 8.30±0.80 57.0±3.0 100.0 Ν
L1448C Per-emb-26 L1448 03:25:38.88 30:44:05.30 8.40±1.50 47.0±7.0 100.0 Y
L1448NW L1448-IRS3C L1448 03:25:35.67 30:45:34.20 1.40±0.10 22.0±1.0 100.0 Ν
Per-emb-02 Barnard 1 03:32:17.92 30:49:47.80 0.90±0.07 27.0±1.0 100.0 Ν
Per-emb-05 (c) 03:31:20.94 30:45:30.20 1.30±0.10 32.0±2.0 100.0 Ν
Per-emb-08 IC348 03:44:43.98 32:01:35.20 2.60±0.50 43.0±6.0 100.0 Ν
Per-emb-18 IRAS7 NGC1333 03:29:11.27 31:18:31.10 2.80±1.70 59.0±12.0 100.0 Ν
Per-emb-22 L1448-IRS2 L1448 03:25:22.41 30:45:13.30 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 31:21:57.1I 23.20±3.00 128.0±23.0 128.0 Ν
Per-emb-62 IC348 03:44:12.98 32:01:35.4I 1.80±0.40 378.0±29.0 378.0 Ν
SVS13A Per-emb-44 NGC1333 03:29:03.76 31:16:03.70/I 32.50±7.10 188.0±9.0 188.0 Υ
SVS13B NGC1333 03:29:03.08 31:15:51.70 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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.