Table 5
Source centres (ra,dec), inclination i, PA, and systemic velocity υLSR for all discs in the analysed sample.
| RA | Dec | Inc [deg] | PA [deg] | υlsr [m s−1] | |
|---|---|---|---|---|---|
| CIDA 9 A | 05h05m22.8260 | +25d31m30.5550 |  |
 |
 |
| DH Tau A | 04h29m41.5610 | +26d32m57.7442 |  |
 |
 |
| DK Tau A | 04h30m44.2509 | +26d01m24.2994 |  |
 |
 |
| DK Tau B | 04h30m44.4048 | +26d01m23.1589 |  |
 |
 |
| HK Tau A | 04h31m50.5769 | +24d24m17.3400 |  |
 |
 |
| HK Tau B | 04h31m50.6122 | +24d24m15.1045 |  |
 |
~6000 |
| HN Tau A | 04h33m39.3782 | +17d51m51.9698 |  |
 |
 |
| RW Aur A | 05h07m49.5716 | +30d24m04.7380 |  |
 |
~6000 |
| RW Aur B | 05h07m49.4597 | +30d24m04.3309 |  |
 |
~5200 |
| UZ Tau E | 04h32m43.0742 | +25d52m30.6460 |  |
 |
 |
| UZ Tau Wa | 04h32m42.8236 | +25d52m31.1959 |  |
 |
 |
| UZ Tau Wb | 04h32m42.8159 | +25d52m30.8347 |  |
 |
 |
| V710 Tau A | 04h31m57.8081 | +18d21m37.6092 |  |
 |
 |
Notes. The PA is defined as the angle to the redshifted disc major-axis counting from north to east. The target centres for circumsecondary discs and for the disc of RW Aur A were estimated through the CASA tool imfit. The disc inclination and PA of HK Tau B are those reported in McCabe et al. (2011). The systemic velocity of HK Tau B is estimated from the spectrum (see Fig. A.1), while υlsr of RW Aur discs are assumed from Rodriguez et al. (2018). All other parameters were estimated using the eddy tool.
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