Table B.1
Observed integrated CO 3–2 intensity in a 40′′ beam from the JCMT and APEX, and CO outflow force, FCO.
| Source | rmsa |
|
|
Δνmaxb | FCOc | Reference |
| (mK) | (K) | (K km s-1) | (km s-1) | (M⊙ yr-1 km s-1) | ||
|
|
||||||
| L1448-MM | 0.07 | 6.2 | 120 | 134 | 9.6(−5) | 1, 2, 3 |
| NGC 1333-IRAS2A | 0.11 | 14.3 | 106 | 26 | 2.4(−4) | 3 |
| NGC 1333-IRAS4A | 0.06 | 12.7 | 69 | 34 | 2.3(−4) | 3 |
| NGC 1333-IRAS4B | 0.04 | 9.9 | 46 | 24 | 1.2(−4) | 3 |
| L1527 | 0.17 | 12.4 | 29 | 7 | 1.6(−4) | 1, 4 |
| Ced110-IRS4 | 0.77 | 9.8 | 50 | 7 | 9.6(−5) | 5 |
| BHR71 | 0.05 | 13.2 | 85 | 144 | 2.6(−3) | 6 |
| IRAS 15398 | 0.15 | 8.8 | 25 | 10 | 3.9(−5) | 5 |
| L483d | 0.05 | 7.7 | 33 | 17 | 1.5(−5) | 1 |
| Ser SMM1 | 0.10 | 15.5 | 133 | 46 | 1.1(−4) | 7 |
| Ser SMM4 | 0.09 | 25.8 | 142 | 43 | 1.1(−4) | 7 |
| Ser SMM3 | 0.09 | 18.3 | 191 | 39 | 3.8(−5) | 7 |
| L723 | 0.07 | 9.8 | 64 | 29 | 6.0(−5) | 1 |
| B335d | 0.38 | 9.1 | 44 | 10 | 2.4(−5) | 1 |
| L1157 | 0.08 | 8.0 | 58 | 43 | 1.5(−4) | 8 |
|
|
||||||
| NGC 1333-IRAS3 | 0.09 | 17.7 | 116 | 36 | 6.2(−4) | 2, 3 |
| L1489 | 0.54 | 5.7 | 21 | 5 | 1.4(−5) | 4 |
| L1551-IRS5 | 0.08 | 8.2 | 56 | 26 | 2.2(−3) | 2, 4 |
| TMR1 | 0.12 | 6.2 | 13 | 7 | 6.6(−6) | 1, 4 |
| TMC1A | 0.13 | 3.8 | 35 | 17 | 8.7(−6) | 1, 4 |
| TMC1 | 0.14 | 3.7 | 19 | 14 | 2.6(−6) | 1, 4 |
| HH46-IRS | 0.55 | 19.0 | 90 | 17 | 1.7(−4) | 5 |
| IRAS 12496 | 0.42 | 12.5 | 85 | 24 | e | |
| GSS30-IRS1 | 0.10 | 29.3 | 120 | 17 | e | |
| Elias29 | 0.09 | 19.8 | 78 | 17 | 2.1(−6) | 1, 9 |
| IRS63 | 0.13 | 11.5 | 31 | 12 | 6.4(−7) | 1, 9 |
| RNO91 | 0.09 | 8.1 | 23 | 12 | 4.2(−6) | 9 |
| RCrA-IRS5A | 0.35 | 34.9 | 174 | 17 | e | |
| HH100-IRS | 0.39 | 23.4 | 120 | 17 | 4.4(−7) | 5 |
|
|
||||||
Notes.
CO outflow force obtained from the literature. All values have been scaled to the distances used here. When multiple values were available, the average is used.
No values available in the literature. IRAS 12496 has an outflow seen nearly face-on, and so any value for FCO is uncertain at best; GSS30-IRS1 is located in a crowded region of Ophiuchus, and it is not possible to determine which outflow the source may be driving in single-dish CO 3–2 maps (van der Marel et al., in prep.).
References. (1) Bontemps et al. (1996); (2) Cabrit & Bertout (1992); (3) Curtis et al. (2010); (4) Hogerheijde et al. (1998); (5) van Kempen et al. (2009b); (6) Bourke et al. (1997); (7) Dionatos et al. (2010); (8) Bachiller et al. (2001); (9) van der Marel et al. (in prep.).
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