Table 1
Source parameters used for Keplerian masking and computing the gas radii.
| Name | Distance | M★ | Log10(L★) | Vsys | Vint | PA | Inc. | Ref. |
|---|---|---|---|---|---|---|---|---|
| (pc) | (M⊙) | (L⊙) | (km s−1) | (km s−1) | (º) | (º) | ||
| AB Aur | 155.0 | 2.4 | 1.7 | 5.8 | 1.5 | −36 | 23 | Tang et al. (2017) |
| AK Sco | 139.2 | 1.7 | 0.8 | 5.4 | 2.5 | 128 | 109 | Czekala et al. (2015) |
| BH Cep | 323.9 | 1.5 | 0.8 | – | – | – | – | |
| BO Cep | 367.9 | 1.4 | 0.6 | −11.6 | 2.0 | −60 | 30 | This work |
| CQ Tau | 148.6 | 1.5 | 0.8 | 6.2 | 1.5 | −50 | 35 | Wölfer et al. (2021) |
| HD 9672 | 57.1 | 1.9 | 1.2 | 2.8 | 2.5 | 73 | 81 | Hughes et al. (2017) |
| HD 31648 | 155.2 | 1.9 | 1.2 | 5.1 | 1.5 | 148 | 37 | Liu et al. (2019) |
| HD 34282 | 311.5 | 1.5 | 1.0 | −2.4 | 1.0 | 65 | 60 | van der Plas et al. (2017) |
| HD 36112 | 155.0 | 1.6 | 0.9 | 6.0 | 1.5 | −60 | 21 | Isella et al. (2010) |
| HD 58647 | 302.2 | 4.1 | 2.5 | – | – | – | – | |
| HD 97048 | 184.1 | 2.8 | 1.8 | 4.6 | 1.5 | −176 | 41 | Walsh et al. (2016) |
| HD 100453 | 103.6 | 1.6 | 0.8 | 5.2 | 1.5 | −145 | 35 | Rosotti et al. (2020) |
| HD 100546 | 108.0 | 2.1 | 1.3 | 5.6 | 1.5 | −140 | 42 | Pineda et al. (2019) |
| HD 104237 | 106.5 | 1.9 | 1.3 | 4.8 | 2.0 | 110 | 20 | This work |
| HD 135344B | 134.4 | 1.5 | 0.7 | 7.1 | 1.5 | −62 | 10 | Cazzoletti et al. (2018) |
| HD 139614 | 133.1 | 1.6 | 0.8 | 6.8 | 1.5 | −100 | 18 | Muro-Arena et al. (2020) |
| HD 141569 | 111.1 | 2.1 | 1.4 | 6.4 | 2.0 | −175 | 53 | White et al. (2016) |
| HD 142527 | 158.5 | 2.2 | 1.4 | 3.6 | 1.5 | 26 | 27 | Kataoka et al. (2016) |
| HD 142666 | 145.5 | 1.8 | 1.1 | 4.1 | 1.5 | 18 | 62 | Huang et al. (2018) |
| HD 163296 | 100.6 | 1.9 | 1.2 | 5.9 | 2.0 | −137 | 47 | Huang et al. (2018) |
| HD 169142 | 114.4 | 1.6 | 0.8 | 6.9 | 0.8 | −175 | 13 | Fedele et al. (2017) |
| HD 176386 | 154.3 | 2.6 | 1.6 | – | – | – | – | |
| HD 200775 | 352.4 | 7.0 | 3.4 | – | – | – | – | |
| HD 245185 | 410.4 | 2.2 | 1.5 | 13.1 | 2.0 | 100 | 30 | This work |
| HD 290764 | 397.1 | 2.0 | 1.3 | 9.5 | 2.0 | 70 | 30 | Kraus et al. (2017) |
| HR 5999 | 157.8 | 3.2 | 2.0 | – | – | – | – | |
| KK Oph | 221.1 | 1.5 | 0.7 | – | – | – | – | |
| MWC 297 | 407.8 | 20.0 | 4.8 | – | – | – | – | |
| SV Cep | 340.3 | 2.0 | 1.3 | – | – | – | – | |
| TY CrA | 158.3 | 2.6 | 1.6 | – | – | – | – | |
| V718 Sco | 153.9 | 1.7 | 1.1 | 8.4 | 1.5 | – | – | |
| V892 Tau | 152.5 | 6.0 | 0.1 | 8.4 | 4.0 | −60 | 55 | Long et al. (2021) |
| VV Ser | 403.4 | 3.6 | 2.3 | – | – | – | – | |
| XY Per | 419.2 | 3.7 | 2.3 | – | – | – | – | |
| ZCMa | 229.7 | 3.8 | 2.3 | – | – | – | – |
Notes. The distances, masses and luminosities are from Guzmán-Díaz et al. (2021), except for KK Oph, V892 Tau and Z CMa which are from Vioque et al. (2018). The distance and luminosity of V892 Tau are also taken from Vioque et al. (2018), but the stellar mass is from Long et al. (2021). The PA and inclination references are given in the last column. The PA is defined as the angle in the clockwise direction between north and the blueshifted side of the disk. For three disks the position angle and inclination were determined by eye based on the 12CO Keplerian mask. Vsys and Vint are respectively the system velocity of the disk and the internal velocity which is the range in velocities due to emission from different layers in the disk, as determined by the data.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.