Table E.3.
Source sample from Alonso-Martínez et al. (2017), hereafter abbreviated as AM17.
| Source | Cloud | Class | RA(J2000) (a) | Dec(J2000) (a) | D | Ṁout([O I]63) | Ṁacc(g) | Main Refs. |
|---|---|---|---|---|---|---|---|---|
| (h m s) | (° ′ ″) | (pc) | (M⊙ yr−1) | (M⊙ yr−1) | ||||
| AA Tau | Tau | II | 04 34 55.42 | +24 28 53.16 | 140 | 1.29 ± 0.37 × 10−9(b) | 2.51 × 10−8 | AM17 |
| CW Tau | Tau | II | 04 14 17.00 | +28 10 57.80 | 140 | 6.68 ± 1.72 × 10−9(b) | 5.27 × 10−8 | AM17 |
| DF Tau | Tau | II | 04 27 03.08 | +25 42 23.30 | 140 | 3.74 ± 0.37 × 10−9(d) | 10.05 × 10−8 | AM17 |
| DG Tau | Tau | II | 04 27 04.70 | +26 06 16.30 | 140 | 1.01 ± 0.04 × 10−7(b) | 2.53 × 10−7 | AM17 |
| DL Tau | Tau | II | 04 33 39.06 | +25 20 38.23 | 140 | 1.35 ± 0.12 × 10−9(d) | 2.48 × 10−8 | AM17 |
| DO Tau | Tau | II | 04 38 28.58 | +26 10 49.44 | 140 | 1.23 ± 0.29 × 10−8(b) | 3.12 × 10−8 | AM17 |
| DP Tau | Tau | II | 04 42 37.70 | +25 15 37.50 | 140 | 8.39 ± 1.23 × 10−9(b) | 0.04 × 10−8 | AM17 |
| DQ Tau | Tau | II | 04 46 53.05 | +17 00 00.20 | 140 | 1.29 ± 0.25 × 10−9(d) | 0.59 × 10−8 | AM17 |
| FS Tau | Tau | II | 04 22 02.18 | +26 57 30.50 | 140 | 3.27 ± 0.12 × 10−8(b) | (2−3)×10−7(c) | AM17 |
| GG Tau | Tau | II | 04 32 30.35 | +17 31 40.60 | 140 | 3.25 ± 0.74 × 10−9(b) | 7.95 × 10−8 | AM17 |
| Haro 6-13 | Tau | II | 04 32 15.41 | +24 28 59.70 | 140 | 3.12 ± 0.86 × 10−9(b) | 2.88 × 10−8(e) | AM17 |
| HL Tau | Tau | II | 04 31 38.44 | +18 13 57.65 | 140 | 3.14 ± 0.03 × 10−8(d) | 0.35 × 10−8 | AM17 |
| HN Tau | Tau | II | 04 33 39.35 | +17 51 52.37 | 140 | 3.68 ± 0.55 × 10−9(b) | 0.49 × 10−8 | AM17 |
| IRAS04385+2550 (f) | Tau | II | 04 41 38.82 | +25 56 26.75 | 140 | 4.72 ± 0.74 × 10−9(b) | 7.76 × 10−9(e) | AM17 |
| RW Aur | Tau | II | 05 07 49.54 | +30 24 05.07 | 140 | 1.43 ± 0.28 × 10−8(b) | (0.034−1.6)×10−6(c) | AM17 |
| SU Aur | Tau | II | 04 55 59.38 | +30 34 01.56 | 140 | 8.03 ± 0.74 × 10−9(b) | 18.03 × 10−8 | AM17 |
| T Tau | Tau | II | 04 21 59.43 | +19 32 06.37 | 140 | 1.12 ± 0.02 × 10−6(b) | 2.36 × 10−7 | AM17 |
| UY Aur | Tau | II | 04 51 47.38 | +30 47 13.50 | 140 | 2.24 ± 0.09 × 10−8(b) | 6.74 × 10−8 | AM17 |
| UZ Tau | Tau | II | 04 32 42.89 | +25 52 32.60 | 140 | 2.76 ± 0.86 × 10−9(d) | 0.45 × 10−8 | AM17 |
| V773 Tau | Tau | II | 04 14 12.92 | +28 12 12.45 | 140 | 5.57 ± 0.74 × 10−9(b) | 11.95 × 10−8 | AM17 |
| XZ Tau | Tau | II | 04 31 39.48 | +18 13 55.70 | 140 | 5.90 ± 0.36 × 10−8(b) | 0.71 × 10−8 | AM17 |
Notes. Sources were selected with the following selection criteria: (a) Class II outflow sources (see Table 2 in Howard et al. 2013; b) Ṁacc is given in Table A.1 in AM17; (c) integrated [O I]63 line fluxes over 3 × 3 spaxels are stated with error margins in Table C.3.
Coordinates from Howard et al. (2013).
Accretion rates from Podio et al. (2012).
Calculated via Eq. (3) from the given line [O I]63 fluxes stated in Table 1 in Aresu et al. (2014).
Accretion rates are calculated from the U-band excess (see description in Alonso-Martínez et al. 2017).
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