Table 5
Position angle, inclination, major axis sizes, and estimates of the mean deconvolved major axis sharpness of the millimeter data.
| Sources | PA | iAxisRatio | B7 | B6 | B4 | Optical-NIR | Δr∕r |
|---|---|---|---|---|---|---|---|
| (°) | (°) | (′′) | (′′) | (′′) | (′′) | ||
| Tau 042021 | −16 | >85 | 4.10 ± 0.01 | 3.76 ± 0.02 | 3.67 ± 0.01 | 5.0 | 0.6 ± 0.2 |
| HH 30 | 121 | >85 (a) | 1.85 ± 0.01 | 1.82 ± 0.02 | 1.73 ± 0.01 | 3.1 | 0.2 ± 0.1 |
| IRAS 04302 | 175 | >84 | 3.15 ± 0.03 | 2.84 ± 0.01 | 0.7 ± 0.1 | ||
| HK Tau B | 41 | >83 | 0.99 ± 0.01 | 0.99 ± 0.01 | 1.3 | 0.2 ± 0.1 | |
| HV Tau C | 108 | >80 | 1.20 ± 0.01 | 1.18 ± 0.01 | 0.8 | 0.5 ± 0.2 | |
| IRAS 04200 | 129 | 69 ± 2 | 1.00 ± 0.01 | 0.85 ± 0.01 | 1.0 ± 0.4 | ||
| Haro 6-5B | 145 | 74 ± 2 | 2.06 ± 0.01 | 1.74 ± 0.01 | 2.3 | 0.8 ± 0.3 (†) | |
| IRAS 04158 | 92 | 62 ± 3 | 7.47 ± 0.03 | 13.6 | |||
| Oph 163131 | 49 | >80 | 2.50 ± 0.01 | 2.6 | 0.7 ± 0.2 | ||
| ESO-Hα 569 | 144 | >64 | 1.88 ± 0.04 | 2.0 | 0.9 ± 0.2 | ||
| ESO-Hα 574 | 141 | >69 | 1.35 ± 0.04 | 1.2 | 0.7 ± 0.2 | ||
| HH 48 NE | 75 | >68 | 1.72 ± 0.03 | 1.3 | 0.4 ± 0.1 |
Notes. For each source, the errors in the millimeter sizes correspond to one tenth of the beam width in the major axis direction. When possible, the Δr∕r ratios correspond to their averaged values between the band 7 and band 4. All are deconvolved by the beam. We also indicate an estimate of the inclination inferred from the millimetric mean axis ratio. These are lower limits when the disks are not resolved along their minor axis in all bands by more than two beams, or when the measured inclination is too high not to be influenced by the physical vertical extent of the disk. (†) Δr∕r of the band 7 only.
References. (a)Louvet et al. (2018).
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