Table 1
Source parameters.
| Source | RA | Dec | Da | νLSR b | Lbolc | T bol c | M env d | F CO e |
| (h m s) | (°′′′) | (pc) | (km s-1) | (L⊙) | (K) | (M⊙) | (M⊙ yr-1 km s-1) | |
|
|
||||||||
| L1448-MM | 03 25 38.9 | +30 44 05.4 | 235 | +5.2 | 9.0 | 46 | 3.9 | 3.7×10-3 |
| NGC 1333-IRAS2A | 03 28 55.6 | +31 14 37.1 | 235 | +7.7 | 35.7 | 50 | 5.1 | 7.4×10-3 |
| NGC 1333-IRAS4A | 03 29 10.5 | +31 13 30.9 | 235 | +7.2 | 9.1 | 33 | 5.2 | 2.1×10-3 |
| NGC 1333-IRAS4B | 03 29 12.0 | +31 13 08.1 | 235 | +7.4 | 4.4 | 28 | 3.0 | 2.2×10-4 |
| L1527 | 04 39 53.9 | +26 03 09.8 | 140 | +5.9 | 1.9 | 44 | 0.9 | 4.4×10-4 |
| Ced110-IRS4 | 11 06 47.0 | −77 22 32.4 | 125 | +4.2 | 0.8 | 56 | 0.2 | − |
| BHR71 | 12 01 36.3 | −65 08 53.0 | 200 | −4.4 | 14.8 | 44 | 3.1 | − |
| IRAS 15398f | 15 43 01.3 | −34 09 15.0 | 130 | +5.1 | 1.6 | 52 | 0.5 | 9.5×10-5 |
| L483 | 18 17 29.9 | −04 39 39.5 | 200 | +5.2 | 10.2 | 49 | 4.4 | 5.9×10-4 |
| Ser-SMM1 | 18 29 49.8 | +01 15 20.5 | 415 | +8.5 | 99.0 | 39 | 52.5 | 3.0×10-3 |
| Ser-SMM3 | 18 29 59.2 | +01 14 00.3 | 415 | +7.6 | 16.6 | 38 | 10.4 | 4.2×10-3 |
| Ser-SMM4 | 18 29 56.6 | +01 13 15.1 | 415 | +8.0 | 6.2 | 26 | 6.9 | 4.8×10-3 |
| L723 | 19 17 53.7 | +19 12 20.0 | 300 | +11.2 | 3.6 | 39 | 1.3 | 2.9×10-3 |
| B335 | 19 37 00.9 | +07 34 09.6 | 250 | +8.4 | 3.3 | 36 | 1.2 | 6.0×10-4 |
| L1157 | 20 39 06.3 | +68 02 15.8 | 325 | +2.6 | 4.7 | 46 | 1.5 | 3.7×10-3 |
|
|
||||||||
| NGC 1333-IRAS3A | 03 29 03.8 | +31 16 04.0 | 235 | +8.5 | 41.8 | 149 | 8.6 | − |
| L1489 | 04 04 43.0 | +26 18 57.0 | 140 | +7.2 | 3.8 | 200 | 0.2 | 1.6×10-4 |
| L1551-IRS5 | 04 31 34.1 | +18 08 05.0 | 140 | +6.2 | 22.1 | 94 | 2.3 | 5.1×10-4 |
| TMR1f | 04 39 13.7 | +25 53 21.0 | 140 | +6.3 | 3.8 | 133 | 0.2 | 2.5×10-5 |
| TMC1Af | 04 39 34.9 | +25 41 45.0 | 140 | +6.6 | 2.7 | 118 | 0.3 | 1.3×10-4 |
| TMC1 | 04 41 12.4 | +25 46 36.0 | 140 | +5.2 | 0.9 | 101 | 0.2 | 4.5×10-4 |
| HH46-IRS | 08 25 43.9 | −51 00 36.0 | 450 | +5.2 | 27.9 | 104 | 4.4 | 1.1×10-3 |
| IRAS 12496 | 12 53 17.2 | −77 07 10.6 | 178 | +3.1 | 35.4 | 569 | 0.8 | − |
| GSS30-IRS1 | 16 26 21.4 | −24 23 04.0 | 125 | +3.5 | 13.9 | 142 | 0.6 | 5.2×10-4 |
| Elias 29 | 16 27 09.4 | −24 37 19.6 | 125 | +4.3 | 14.1 | 299 | 0.3 | 6.4×10-5 |
| Oph-IRS63 | 16 31 35.6 | −24 01 29.6 | 125 | +2.8 | 1.0 | 327 | 0.3 | 1.1×10-5 |
| RNO91 | 16 34 29.3 | −15 47 01.4 | 125 | +0.5 | 2.6 | 340 | 0.5 | 1.0×10-4 |
| RCrA-IRS5A | 19 01 48.0 | −36 57 21.6 | 130 | +5.7 | 7.1 | 126 | 2.0 | − |
| HH100-IRS | 19 01 49.1 | −36 58 16.0 | 130 | +5.6 | 17.7 | 256 | 8.1 | − |
Notes. Sources above the horizontal line are Class 0, sources below are Class I.
Taken from van Dishoeck et al. (2011) with the exception of sources in Serpens, where we use the distance determined using VLBA observations by Dzib et al. (2010).
Obtained from ground-based C18O or C17O observations (Yıldiz et al. 2013) with the exception of IRAS4A for which the value from Kristensen et al. (2012) is more consistent with our data.
Measured using Herschel PACS data from the WISH and DIGIT key programmes (Karska et al. 2014).
Mass within the 10 K radius, determined by Kristensen et al. (2012) from dusty modelling of the sources.
Taken from Yıldiz et al. (2014) for CO 3−2.
The coordinates used in WISH; more accurate SMA coordinates of the sources are 15h43m02
2, −34°09′06.̋8 (IRAS 15398), 04h39m139, +25°53′20.̋6 (TMR1) and 04h39m352, +25°41′44.̋4 (TMC1A; Jørgensen et al. 2009). For IRAS 15398, these coordinates were observed in two settings as part of the OT2 programme OT2_evandish_4.
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