Table E.1.
Source sample from the DIGIT and WISH surveys.
| Source | Cloud | Class (a) | RA(J2000) (b) | Dec(J2000) (b) | D | Ṁout([O I]) | Ṁout(mol) |
 (i) |
Ṁacc(g) | Main Refs. |
|---|---|---|---|---|---|---|---|---|---|---|
| (h m s) | (° ′ ″) | (pc) | (M⊙ yr−1) | (M⊙ yr−1) | (M⊙ yr−1) | |||||
| IRAS03245+3002 | Per | 0 | 03 27 39.09 | +30 13 03.0 | 235 | 6.4 × 10−8 | 4.2 × 10−6 | Mo17 | ||
| L1455-ISR3 | Per | I | 03 28 00.40 | +30 08 01.3 | 235 | 5.0 × 10−8 | 4.7 × 10−8 | Mo17 | ||
| NGC 1333-IRAS 4B | Per | 0 | 03 29 12.04 | +31 13 01.5 | 235 | 1.3 × 10−8 | ∼3.5 × 10−7(k) | 3.7 × 10−2 | 2.9 × 10−6 | Mo17 |
| B1a | Per | I | 03 33 16.66 | 31 07 55.2 | 235 | 1.9 × 10−8 | 3.5 × 10−7 | Mo17 | ||
| L1489 | Tau | I | 04 04 42.9 | +26 18 56.3 | 140 | 2.2 × 10−8 | ∼6.1 × 10−7(e) | 3.6 × 10−2 | 4.9 × 10−7 | Mo17 |
| TMR1 | Tau | I | 04 39 13.9 | +25 53 20.6 | 140 | 1.1 × 10−7 | ∼4.1 × 10−7(e) | 2.6 × 10−1 | 4.9 × 10−7 | Mo17 |
| TMC1A | Tau | I | 04 39 35.0 | +25 41 45.5 | 140 | 3.3 × 10−7 | ∼7.3 × 10−7(e) | 4.5 × 10−1 | 3.5 × 10−7 | Mo17 |
| L1527 | Tau | 0 | 04 39 53.9 | +26 03 09.8 | 140 | 1.8 × 10−7 | ∼4.5 × 10−6(e) | 4.0 × 10−2 | 1.2 × 10−6 | Mo17 |
| TMC1 | Tau | I | 04 41 12.7 | +25 46 35.9 | 140 | 1.5 × 10−7 | ∼1.6 × 10−6(e) | 9.4 × 10−2 | 1.2 × 10−7 | Mo17 |
| IRAM04191+1522 | Tau | 0 | 04 21 56.9 | +15 29 45.9 | 140 | 2.4 × 10−8 | 7.1 × 10−8 | Mo17 | ||
| Ced110-IRS4 | ChaI | 0 | 11 06 47.0 | −77 22 32.4 | 150 | 1.3 × 10−7 | ∼3.3 × 10−7(e) | 3.4 × 10−1 | 5.2 × 10−7 | Mo17 |
| IRAS15398-3359 | Lup | 0 | 15 43 01.29 | −34 09 15.4 | 130 (c) | 3.0 × 10−7 | ∼3.2 × 10−6(e) | 9.4 × 10−2 | 1.0 × 10−6 | Mo17 |
| GSS30 IRS1 | Oph | I | 16 26 21.48 | −24 23 04.2 | 125 | 5.1 × 10−7 | ∼1.3 × 10−5(e) | 3.9 × 10−3 | 1.8 × 10−6 | Mo17 |
| WL12 | Oph | I | 16 26 44.2 | −24 34 48.4 | 125 | 7.9 × 10−8 | 2.1 × 10−7 | Mo17 | ||
| Elias29 | Oph | I | 16 27 09.36 | −24 37 18.4 | 125 | 4.0 × 10−7 | ∼1.6 × 10−6(e) | 2.5 × 10−1 | 1.8 × 10−6 | Mo17 |
| IRS44 | Oph | I | 16 27 28.1 | −24 39 33.4 | 125 | 4.8 × 10−8 | 6.6 × 10−7 | Mo17 | ||
| IRS46 | Oph | I | 16 27 29.4 | −24 39 16.1 | 125 | 1.5 × 10−8 | 6.5 × 10−8 | Mo17 | ||
| IRS63 | Oph | I | 16 31 35.76 | −24 01 29.2 | 125 | 3.3 × 10−8 | ∼1.3 × 10−5(f) | 1.3 × 10−7 | Mo17 | |
| L483 MM | Aqu | 0 | 18 17 29.9 | −04 39 39.5 | 200 (c) | 1.1 × 10−7 | ∼1.1 × 10−5(e) | 1.0 × 10−2 | 6.6 × 10−6 | Mo17 |
| Ser-SMM1 | Ser | 0 | 18 29 49.56 | +01 15 21.9 | 436 | 4.0 × 10−7 | ∼2.2 × 10−5(e) | 1.8 × 10−2 | 7.1 × 10−5 | Mo17 |
| Ser-SMM4 | Ser | 0 | 18 29 56.7 | +01 13 17.2 | 436 | 1.8 × 10−6 | ∼2.6 × 10−5(e) | 6.9 × 10−2 | 4.4 × 10−6 | Mo17 |
| Ser-SMM3 | Ser | 0 | 18 29 59.3 | +01 14 01.7 | 436 | 1.1 × 10−6 | ∼3.9 × 10−5(e) | 2.8 × 10−2 | 1.2 × 10−5 | Mo17 |
| L723 MM | Core | 0 | 19 17 53.7 | +19 12 20.0 | 300 (c) | 1.3 × 10−8 | ∼1.5 × 10−5(e) | 8.7 × 10−4 | 2.3 × 10−6 | Mo17 |
| B335 | Core | 0 | 19 37 00.9 | +07 34 09.6 | 106 (d) | 2.5 × 10−8 | ∼1.0 × 10−7(j) | 2.5 × 10−1 | 2.1 × 10−6 | Mo17 |
| L1157 | Core | 0 | 20 39 06.3 | +68 02 16.0 | 325 (d) | 3.3 × 10−8 | ∼4.5 × 10−7(k) | 7.3 × 10−2 | 3.0 × 10−6 | Mo17 |
Notes. We took 25 sources (13 Class 0 and 12 Class I) from Table A.7 in Mottram et al. (2017), hereafter abbreviated as Mo17, with the following selection criteria: (a) Ṁacc and Ṁout are given in Table A.7; (b) sources are not part of the spatially resolved Nisini et al. (2015) sample, which were analysed in much more detail; (c) flat sources are excluded (IRAS03301+3111, IRAS12496, RNO91); (d) we excluded RCRA IRS5A, RCrA-I7A, and RCrA-I7B since they are ambiguously classified.
Classification from Nisini et al. (2002), Green et al. (2013), Karska et al. (2013), and Yang et al. (2018).
Coordinates from Karska et al. (2013).
Yıldız et al. (2015) from CO J = 6–5 observations; the listed values are the sum of the mass-loss rates of both lobes.
Tanabe et al. (2019) from CO J = 1–0 observations, i.e. rather entrained material.
From Mottram et al. (2017) we adopt their method calculating the mass-accretion rates listed in Tables 5 and 6.
Yıldız et al. (2015) from CO J = 3–2 observations; the listed values are the sum of the mass-loss rates of both lobes. As stated therein, CO J = 3–2 traces entrained material.
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