Table E.2.
Source sample from the WILL survey.
| Source (a) | Cloud | Class | RA(J2000) | Dec(J2000) | D | Ṁout([O I]63) | Ṁout(mol)(b) | Ṁacc(c) | Main Refs. |
|---|---|---|---|---|---|---|---|---|---|
| (h m s) | (° ′ ″) | (pc) | (M⊙ yr−1) | (M⊙ yr−1) | (M⊙ yr−1) | ||||
| AQU 01 | Aqu | 0 | 18 29 03.82 | −01 39 01.5 | 436 | 8.3 × 10−8 | 8.5 × 10−5 | 1.7 × 10−6 | Mo17 |
| AQU 02 | Aqu | 0 | 18 29 08.60 | −01 30 42.8 | 436 | 8.2 × 10−8 | 1.3 × 10−5 | 5.9 × 10−6 | Mo17 |
| CRA 01 | CrA | 0 | 19 02 58.67 | −37 07 35.9 | 130 | 1.2 × 10−7 | 2.3 × 10−6 | 1.6 × 10−6 | Mo17 |
| OPH 02 | Oph | I | 16 32 00.99 | −24 56 42.6 | 125 | 5.2 × 10−8 | 2.5 × 10−8 | 1.1 × 10−6 | Mo17 |
| PER 01 | Per | 0 | 03 25 22.32 | +30 45 13.9 | 235 | 3.4 × 10−7 | 8.1 × 10−5 | 2.9 × 10−6 | Mo17 |
| PER 02 | Per | 0 | 03 25 36.49 | +30 45 22.2 | 235 | 7.8 × 10−7 | – | 6.0 × 10−6 | Mo17 |
| PER 04 | Per | 0 | 03 26 37.47 | +30 15 28.1 | 235 | 5.3 × 10−8 | 7.1 × 10−7 | 7.6 × 10−7 | Mo17 |
| PER 05 | Per | I | 03 28 37.09 | +31 13 30.8 | 235 | 2.8 × 10−8 | 1.2 × 10−7 | 1.4 × 10−6 | Mo17 |
| PER 06 | Per | I | 03 28 57.36 | +31 14 15.9 | 235 | 1.6 × 10−7 | – | 9.2 × 10−7 | Mo17 |
| PER 07 | Per | 0 | 03 29 00.55 | +31 12 00.8 | 235 | 1.2 × 10−7 | 3.8 × 10−6 | 4.6 × 10−7 | Mo17 |
| PER 08 | Per | I | 03 29 01.56 | +31 20 20.6 | 235 | 1.1 × 10−6 | 1.4 × 10−5 | 2.2 × 10−6 | Mo17 |
| PER 14 | Per | I | 03 30 15.14 | +30 23 49.4 | 235 | 4.6 × 10−8 | 3.7 × 10−6 | 2.4 × 10−7 | Mo17 |
| PER 15 | Per | 0 | 03 31 20.98 | +30 45 30.1 | 235 | 2.1 × 10−8 | 2.4 × 10−6 | 1.1 × 10−6 | Mo17 |
| PER 16 | Per | 0 | 03 32 17.96 | +30 49 47.5 | 235 | 2.6 × 10−8 | 7.6 × 10−6 | 7.4 × 10−7 | Mo17 |
| PER 17 | Per | I | 03 33 14.38 | +31 07 10.9 | 235 | 1.4 × 10−8 | 1.5 × 10−5 | 2.3 × 10−8 | Mo17 |
| PER 18 | Per | 0 | 03 33 16.44 | +31 06 52.5 | 235 | 1.8 × 10−7 | 3.4 × 10−6 | 3.4 × 10−7 | Mo17 |
| PER 19 | Per | I | 03 33 27.29 | +31 07 10.2 | 235 | 1.8 × 10−7 | 1.7 × 10−6 | 1.4 × 10−7 | Mo17 |
| PER 21 | Per | 0 | 03 43 56.84 | +32 03 04.7 | 235 | 8.6 × 10−8 | 7.8 × 10−6 | 1.2 × 10−6 | Mo17 |
| PER 22 | Per | 0 | 03 44 43.96 | +32 01 36.2 | 235 | 1.0 × 10−7 | 1.5 × 10−6 | 1.6 × 10−6 | Mo17 |
| SERS 01 | Serp | 0 | 18 29 37.70 | −01 50 57.8 | 436 | 2.8 × 10−7 | 1.8 × 10−5 | 1.1 × 10−5 | Mo17 |
| TAU 01 | Tau | I | 04 19 58.40 | +27 09 57.0 | 140 | 7.6 × 10−8 | 1.7 × 10−6 | 2.0 × 10−7 | Mo17 |
| TAU 02 | Tau | I | 04 21 11.40 | +27 01 09.0 | 140 | 1.1 × 10−8 | 2.1 × 10−7 | 6.1 × 10−8 | Mo17 |
| TAU 04 | Tau | I | 04 27 02.60 | +26 05 30.0 | 140 | 4.5 × 10−8 | 7.1 × 10−7 | 1.8 × 10−7 | Mo17 |
| TAU 06 | Tau | I | 04 27 57.30 | +26 19 18.0 | 140 | 9.6 × 10−9 | 1.8 × 10−7 | 7.3 × 10−8 | Mo17 |
| W40 02 | W40 | 0 | 18 31 10.36 | −02 03 50.4 | 436 | 5.4 × 10−6 | 1.0 × 10−5 | 2.1 × 10−5 | Mo17 |
| W40 07 | W40 | 0 | 18 32 13.36 | −01 57 29.6 | 436 | 5.4 × 10−8 | 6.5 × 10−6 | 2.3 × 10−6 | Mo17 |
Notes. We only took the 26 (15 Class 0 and 11 Class I) outflow sources, for which Ṁacc is presented in Table A.7 in Mo17.
Source names adopted from Mottram et al. (2017).
Calculated via the same method presented in Yıldız et al. (2015) but based on low-J CO observations; that is, CO J = 3–2 measuring the entrained material.
From Mottram et al. (2017), we adopted their method calculating the mass-accretion rates listed in Tables 5 and 6.
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