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Table 4
Source parameters.
| Source | d | νLSRa | L bol b | T bol b | M env (10 K) c | n 1000 AU c,d | n 20″ c,e | ||
| [pc] | [km s-1] | [L⊙] | [K] | [M⊙] | [105 cm-3] | [105 cm-3] | |||
|
|
|||||||||
| L1448-MM | 235 | +5.2 | 9.0 | 46 | 3.9 | 39 | 11 | ||
| NGC 1333-IRAS 2A | 235 | +7.7 | 35.7 | 50 | 5.1 | 17 | 4.0 | ||
| NGC 1333-IRAS 4A | 235 | +7.0 | 9.1 | 33 | 5.6 | 67 | 15 | ||
| NGC 1333-IRAS 4B | 235 | +7.1 | 4.4 | 28 | 3.0 | 57 | 17 | ||
| L1527 | 140 | +5.9 | 1.9 | 44 | 0.9 | 8.1 | 6.0 | ||
| Ced110-IRS4 | 125 | +4.2 | 0.8 | 56 | 0.2 | 3.9 | 2.8 | ||
| BHR71 | 200 | −4.4 | 14.8 | 44 | 2.7 | 18 | 5.4 | ||
| IRAS 15398 | 130 | +5.1 | 1.6 | 52 | 0.5 | 16 | 11 | ||
| L483 mm | 200 | +5.2 | 10.2 | 49 | 4.4 | 5.1 | 2.8 | ||
| Ser-SMM1 | 230 | +8.5 | 30.4 | 39 | 16.1 | 41 | 14 | ||
| Ser-SMM4 | 230 | +8.0 | 1.9 | 26 | 2.1 | 54 | 23 | ||
| Ser-SMM3 | 230 | +7.6 | 5.1 | 38 | 3.2 | 11 | 5.5 | ||
| L723 | 300 | +11.2 | 3.6 | 39 | 1.3 | 8.0 | 2.2 | ||
| B335 | 250 | +8.4 | 3.3 | 36 | 1.2 | 15 | 4.3 | ||
| L1157 | 325 | +2.6 | 4.7 | 46 | 1.5 | 20 | 2.9 | ||
|
|
|||||||||
| L1489 | 140 | +7.2 | 3.8 | 200 | 0.2 | 1.9 | 1.2 | ||
| L1551-IRS5 | 140 | +6.2 | 22.1 | 94 | 2.3 | 12 | 6.4 | ||
| TMR1 | 140 | +6.3 | 3.8 | 133 | 0.2 | 2.1 | 1.2 | ||
| TMC1A | 140 | +6.6 | 2.7 | 118 | 0.2 | 2.2 | 1.3 | ||
| TMC1 | 140 | +5.2 | 0.9 | 101 | 0.2 | 1.8 | 1.2 | ||
| HH46-IRS | 450 | +5.2 | 27.9 | 104 | 4.4 | 12 | 1.1 | ||
| DK Cha | 178 | +3.1 | 35.4 | 569 | 0.8 | 9.2 | 3.7 | ||
| GSS30-IRS1 | 125 | +3.5 | 13.9 | 142 | 0.6 | 1.7 | 1.1 | ||
| Elias 29 | 125 | +4.3 | 14.1 | 299 | 0.3 | 0.8 | 0.6 | ||
| Oph-IRS63 | 125 | +2.8 | 1.0 | 327 | 0.3 | 6.9 | 5.0 | ||
| RNO91 | 125 | +0.5 | 2.6 | 340 | 0.5 | 3.3 | 2.4 | ||
Notes.Sources above the horizontal line are Class 0, sources below are Class I.
(b)
Measured using Herschel-PACS data from the WISH and DIGIT key programmes (Karska et al. 2013; Green et al. 2013).
(c)
Determined from DUSTY modeling of the sources; see Kristensen et al. (2012).
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