Table 1
Sources analyzed in this work and their properties: class, [O i] flux, LX and LFUV, and presence of an optical jet/outflow.
| Name | Class | [O i] 63 μm | [O i] 63 μm | L FUV | L X | Outflow |
| [1e–17 W/m2] | disk only | [1e30 erg/s] | [1e30 erg/s] | [YES/NO] | ||
|
|
||||||
| AATau | II | 2.2 ± 0.2 | 0.60 | 28.821 | 1.24 |
Y |
| BPTau | II | 0.10 ± 0.03 | 58.641 | 1.36 |
N | |
| CITau | II | 3.3 ± 0.5 | 13.321 | 0.19 |
N | |
| CWTau | II | 7.2 ± 0.4 | 0.82 | 111.132 | 2.84 |
Y |
| CXTau | T | 0.7 ± 0.3 | 0.681 | – | N | |
| CYTau | II | 1.2 ± 0.4 | 13.321 | 0.13 |
N | |
| DETau | II | 0.7 ± 0.6 | 30.411 | – | N | |
| DFTau | II | 6.1 ± 0.6 | 9.951 | – | Y | |
| DGTau | II | 134.00 ± 17.0 | 4.70 | 318.042 | 0.55 |
Y |
| DHTau | II | <1.35 | – | 8.46 |
N | |
| DKTau | II | 1.6 ± 0.3 | 18.582 | 0.92 |
N | |
| DLTau | II | 2.2 ± 0.2 | 13.971 | – | Y | |
| DMTau | T | 0.7 ± 0.2 | 58.281 | 2.00 |
N | |
| DNTau | T | 0.6 ± 0.2 | 6.521 | 1.15 |
N | |
| DOTau | II | 7.1 ± 1.0 | 1.45 | 470.601 | 0.24 |
Y |
| DPTau | II | 14.8 ± 1.3 | 0.57 | 96.291 | 0.10 |
Y |
| DQTau | II | 2.1 ± 0.4 | 0.822 | – | N | |
| DSTau | II | 0.9 ± 0.2 | 49.961 | – | N | |
| FFTau | III | <1.01 | – | 0.80 |
N | |
| FMTau | II | 1.0 ± 0.2 | 4.891 | 0.53 |
N | |
| FOTau | T | 1.20 ± 0.5 | – | 0.06 |
N | |
| FQTau | II | <0.92 | – | 0.12 |
N | |
| FSTau-A | II-FS | 35.8 ± 0.5 | – | 3.22 |
Y | |
| FXTau | II | <1.38 | – | 0.50 |
N | |
| GGTau | II | 5.1 ± 0.4 | 10.512 | – | N | |
| GHTau | II | <0.85 | – | 0.11 |
N | |
| GI-KTau | II | 3.1 ± 1.4 | 10.861 | 0.83 |
N | |
| GMAur | T | 2.4 ± 0.5 | 28.241 | 1.60 |
N | |
| GOTau | II | <5.38 | – | 0.25 |
N | |
| HBC358 | III | <1.4 | – | 0.38 |
N | |
| HKTau | II | 3.4 ± 0.2 | – | 0.08 |
N | |
| HLTau | I | 51.3 ± 0.5 | – | 3.84 |
Y | |
| HNTau | II | 4.1 ± 0.2 | 0.56 | 21.291 | 0.32 |
Y |
| HOTau | II | <1.03 | – | 0.05 |
N | |
| Haro6-13 | II | 7.0 ± 0.5 | – | 0.80 |
Y | |
| IPTau | T | 0.6 ± 0.2 | 4.051 | – | N | |
| IQTau | II | 1.5 ± 0.3 | – | 0.42 |
N | |
| IRAS043 | II | 4.9 ± 0.2 | – | 0.40 |
Y | |
| LkCa15 | T | 1.0 ± 0.2 | 4.453 | – | N | |
| RWAur | II | 15.4 ± 0.5 | – | 1.60 |
Y | |
| RYTau | T? | 10.5 ± 0.5 | 3.80 | 1042.561 | 5.52 |
Y |
| SUAur | II | 8.6 ± 0.3 | 2.51 | 127.421 | 9.46 |
Y |
| UYAur | II | 31.4 ± 0.4 | 2.16 | 27.732 | 0.40 |
Y |
| UZTau | II | 4.5 ± 1.4 | – | 0.89 |
Y | |
| V710Tau | II | 1.0 ± 0.6 | – | 1.38 |
N | |
| V773Tau | II | 6.5 ± 0.3 | – | 9.49 |
Y | |
| V819Tau | II | <0.898 | – | 2.44 |
N | |
| XZTau | II | 36.1 ± 0.09 | – | 0.96 |
Y | |
Notes. LX is measured between 0.3 and 10 keV, LFUV is measured between 7 and 10 eV. The oxygen fluxes listed in the fourth column are the estimated disk contribution to the total [O i] flux as explained in Sect. 5.2. The class of the objects is taken from Andrews & Williams (2005), X-ray luminosities between 0.3 and 10 kev are taken from Güdel et al. (2007, 2010), FUV luminosities with superscript 1 are retrieved from Yang et al. (2012) (errors are estimated to be ±30%), while the ones with superscript 2 and 3 are calculated using the accretion luminosity retrieved from Gullbring et al. (1998), and Ingleby et al. (2009) respectively (in this case the error is the one associated with the correlation: 0.38 dex). These values are then scaled by a factor 4.25 to estimate the luminosity in the 6–13.6 eV range. Outflow sources are objects for which extended emission in the optical, associated to a jet, has been observed. The [O i] emission from these objects has not been included in the primary analysis performed in this work.
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