Free Access

Table 1

Catalog information and source properties.

Object RA Dec T bol L bol M env Region Other names
(hms) (°′′) (K) (L) (M)

Per01 03:25:22.32 +30:45:13.9 44 4.5 1.14 L1448 Per-emb 22, L1448 IRS2, IRAS03222+3034, YSO 1
Per02 03:25:36.49 +30:45:22.2 50 10.6 3.17 L1448 Per-emb 33, L1448 N(A), L1448 IRS3, YSO 2
Per03a 03:25:39.12 +30:43:58.2 47 8.4 2.56 L1448 Per-emb 42, L1448 MMS, L1448 C(N), YSO 3
Per04 03:26:37.47 +30:15:28.1 61 1.2 0.29 L1451 Per-emb 25, IRAS03235+3004, YSO 4
Per05 03:28:37.09 +31:13:30.8 85 11.1 0.35 NGC 1333 Per-emb 35, NGC 1333 IRAS1, IRAS03255+3103, YSO 11
Per06 03:28:57.36 +31:14:15.9 85 6.9 0.30 NGC 1333 Per-emb 36, NGC 1333 IRAS2B, YSO 16
Per07 03:29:00.55 +31:12:00.8 37 0.7 0.32 NGC 1333 Per-emb 3, HRF 65, YSO 18
Per08 03:29:01.56 +31:20:20.6 131 16.8 0.86 NGC 1333 Per-emb 54, HH 12, YSO 19
Per09 03:29:07.78 +31:21:57.3 128 23.2 0.24 NGC 1333 Per-emb 50
Per10 03:29:10.68 +31:18:20.6 45 6.9 1.37 NGC 1333 Per-emb 21, HRF 46, YSO 23
Per11b 03:29:12.06 +31:13:01.7 28 4.4 5.42 NGC 1333 Per-emb 13, NGC 1333 IRAS4B, YSO 25
Per12 03:29:13.54 +31:13:58.2 31 1.1 1.30 NGC 1333 Per-emb 14, NGC 1333 IRAS4C, YSO 26
Per13 03:29:51.82 +31:39:06.0 40 0.7 0.51 NGC 1333 Per-emb 9, IRAS03267+3128, YSO 31
Per14 03:30:15.14 +30:23:49.4 88 1.8 0.14 B1-ridge Per-emb 34, IRAS03271+3013
Per15 03:31:20.98 +30:45:30.1 35 1.7 1.29 B1-ridge Per-emb 5, IRAS03282+3035, YSO 32
Per16 03:32:17.96 +30:49:47.5 30 1.1 2.75 B1-ridge Per-emb 2, IRAS03292+3039, YSO 33
Per17c 03:33:14.38 +31:07:10.9 43 0.7 1.20 B1 Per-emb 6, B1 SMM3, YSO 35
Per18c 03:33:16.44 +31:06:52.5 25 1.1 1.22 B1 Per-emb 10, B1 d, YSO 36
Per19 03:33:27.29 +31:07:10.2 93 1.1 0.23 B1 Per-emb 30, B1 SMM11, YSO 40
Per20 03:43:56.52 +32:00:52.8 27 2.3 2.05 IC 348 Per-emb 1, HH 211 MMS, YSO 44
Per21 03:43:56.84 +32:03:04.7 34 2.1 1.88 IC 348 Per-emb 11, IC348 MMS, IC348 SW, YSO 43
Per22 03:44:43.96 +32:01:36.2 43 2.6 0.64 IC 348 Per-emb 8, IC348 a, IRAS03415+3152, YSO 48

Notes. Bolometric temperatures and luminosities are determined including the PACS continuum values; the procedure will be discussed in Mottram et al. (in prep.). Numbered Per-emb names come from Enoch et al. (2009), whereas the numbered YSO names come from Jørgensen et al. (2006) and were subsequently used in Davis et al. (2008). Other source identifiers were compiled using Jørgensen et al. (2007), Rebull et al. (2007), Davis et al. (2008), and Velusamy et al. (2014). Observations obtained in 2011 which overlap with Per03 and Per11 are presented in Lee et al. (2013) and Herczeg et al. (2012), respectively.

(a)

Tabulated values come from Green et al. (2013), where full PACS spectra are obtained. The WILL values for Tbol and Lbol are 48 K and 8.0 L, respectively, within 5% of those of Green et al. (2013).

(b)

Tabulated values come from Karska et al. (2013) and agree within 2% of the values 29 K and 4.3 L obtained here. We prefer to use the previously published values because the pointing of that observation was better centered on the IRAS4B.

(b)

The off-positions of Per17 and Per18 were contaminated by other continuum sources, and therefore the Tbol and Lbol are calculated here without the Herschel/PACS points.

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.