Table B.3
Disk masses derived by millimeter fluxes.
| Object | β | TD | Mdisk | N° photometric points | References |
|---|---|---|---|---|---|
| (K) | (M⊙) | ||||
| HBC 1 | 1.0 | 21 | 7.808 ± 0.887 | 1 | (16) |
| VX Cas | 1.0 | 33 | <0.007 | 1 | (27) |
| V594 Cas | 1.1 | 32 | 0.039 ± 0.001 | 2 | (7) (31) |
| HD 9672 | 0.6 | 39 | 2.920E-4 ± 3.060E-5 | 2 | (24) |
| AB Aur | 1.2 | 40 | 0.009 ± 0.002 | 5 | (1) (2) (3) |
| HD 31648 | 0.9 | 20 | 0.051 ± 4.410E-4 | 6 | (1) (2) (5) (20) |
| UX Ori | 0.8 | 22 | 0.016 ± 0.001 | 2 | (27) (32) |
| HD 34282 | 1.5 | 38 | 0.040 ± 0.004 | 6 | (1) (11) (16) (21) |
| HD 34700 | 1.1 | 28 | 0.008 ± 0.001 | 4 | (8) (11) (22) (23) |
| HD 35187 | 0.5 | 42 | 0.003 ± 1.800E-4 | 3 | (1) (4) |
| CO Ori | 1.0 | 16 | <0.006 | 1 | (8) |
| HD 36112 | 1.5 | 31 | 0.006 ± 1.140E-4 | 3 | (1) (5) |
| HD 245185 | 0.1 | 46 | 0.016 ± 0.003 | 2 | (5) |
| T Ori | 1.0 | 28 | 0.108 ± 0.023 | 1 | (8) |
| CQ Tau | 0.4 | 19 | 0.028 ± 3.410E-4 | 2 | (5) |
| V380 Ori | 1.0 | 33 | 0.041 ± 0.016 | 1 | (34) |
| BF Ori | 1.0 | 25 | 0.005 ± 0.002 | 1 | (8) |
| HD 290764 | 1.0 | 19 | 0.244 ± 0.026 | 1 | (19) |
| V599 Ori | 1.0 | 22 | 0.091 ± 0.007 | 1 | (36) |
| RR Tau | 0.3 | 29 | 0.058 ± 0.005 | 2 | (31) |
| HD 250550 | 1.0 | 38 | <0.085 | 1 | (7) |
| HD 41511 | 0.3 | 16 | 0.019 ± 0.002 | 2 | (2) |
| GSC 1876-0892 | 1.0 | 71 | 19.646 ± 6.445 | 1 | (9) |
| LkHa 208 | 1.0 | 17 | <0.014 | 1 | (27) |
| MWC 137 | 1.2 | 143 | 1.948 ± 0.281 | 6 | (14) |
| VY Mon | 1.9 | 58 | 0.052 ± 0.006 | 5 | (1) (31) |
| LkHa 215 | 1.8 | 70 | 0.061 ± 0.015 | 3 | (14) |
| HD 259431 | 1.0 | 44 | <0.052 | 1 | (14) |
| HT CMa | 1.0 | 33 | <0.180 | 1 | (6) |
| Z CMa | 1.9 | 36 | 1.383 ± 0.017 | 8 | (33) |
| PDS 241 | 1.0 | 172 | 57.362 ± 1.616 | 9 | (28) |
| V388 Vel | 1.9 | 47 | 0.294 ± 0.093 | 3 | (35) |
| HD 76534 | 1.0 | 101 | <0.019 | 1 | (6) |
| PDS 37 | 1.0 | 101 | 15.663 ± 3.040 | 1 | (29) |
| HD 97048 | 1.6 | 24 | 0.094 ± 0.007 | 3 | (25) (26) |
| HD 100453 | 1.0 | 17 | 0.025 ± 0.002 | 1 | (4) |
| HD 100546 | 1.3 | 13 | 0.061 ± 0.003 | 4 | (4) (6) (10) |
| HD 104237 | 1.0 | 19 | 0.008 ± 0.002 | 1 | (6) |
| HD 135344B | 1.4 | 30 | 0.013 ± 0.002 | 3 | (1) (11) |
| HD 135344 | 1.7 | 27 | 0.011 ± 0.009 | 3 | (10) |
| HD 139614 | 0.6 | 29 | 0.022 ± 0.001 | 4 | (4) (11) |
| HD 141569 | 1.0 | 46 | 1.460E-4 ± 1.570E-5 | 3 | (1) (5) |
| HD 142666 | 0.5 | 30 | 0.013 ± 0.001 | 3 | (1) (11) |
| HD 142527 | 0.3 | 19 | 0.211 ± 5.810E-5 | 2 | (5) |
| HD 143006 | 1.0 | 15 | 0.032 ± 4.940E-5 | 1 | (12) |
| HD 144432 | 1.6 | 6 | 0.021 ± 0.002 | 3 | (4) |
| HR 5999 | 0.0 | 15 | 0.008 ± 2.190E-4 | 2 | (1) (13) |
| HD 150193 | 0.6 | 40 | 0.004 ± 0.001 | 4 | (1) (2) (4) |
| AK Sco | 0.3 | 27 | 0.003 ± 7.350E-6 | 4 | (4) (5) |
| V921 Sco | 1.0 | 215 | 0.360 ± 0.047 | 1 | (7) |
| HD 158643 | 1.0 | 28 | 3.780E-4 ± 4.530E-5 | 1 | (13) |
| HD 163296 | 0.4 | 34 | 0.034 ± 0.001 | 8 | (14) |
| HD 169142 | 1.2 | 31 | 0.010 ± 3.090E-4 | 5 | (1) (4) (5) |
| MWC 297 | 0.0 | 200 | 0.029 ± 0.001 | 3 | (1) (6) |
| VV Ser | 0.0 | 35 | 9.540E-4 ± 2.730E-4 | 2 | (31) |
| V431 Sct | 1.0 | 101 | 0.225 ± 0.062 | 1 | (6) |
| PDS 520 | 1.0 | 16 | 0.162 ± 0.021 | 1 | (30) |
| AS 310 | 1.0 | 215 | 0.768 ± 0.050 | 1 | (6) |
| HD 176386 | 1.0 | 33 | 0.121 ± 0.010 | 1 | (15) |
| TY CrA | 1.0 | 38 | <0.017 | 1 | (17) |
| HD 179218 | 1.4 | 24 | 0.029 ± 0.003 | 2 | (16) |
| WW Vul | 1.0 | 23 | 0.016 ± 0.001 | 1 | (4) |
| V1685 Cyg | 1.0 | 101 | 0.255 ± 0.033 | 1 | (7) |
| V1686 Cyg | 1.0 | 16 | <0.040 | 1 | (8) |
| V1478 Cyg | 0.0 | 35 | 12.973 ± 0.349 | 2 | (1) |
| HD 200775 | 1.0 | 71 | <0.015 | 1 | (17) |
| HD 235495 | 1.0 | 33 | 0.038 ± 0.005 | 1 | (18) |
| V361 Cep | 1.0 | 71 | <0.032 | 1 | (7) |
| V373 Cep | 1.0 | 44 | <0.051 | 1 | (33) |
| AS 477 | 1.0 | 33 | <0.051 | 1 | (7) |
| SV Cep | 1.0 | 23 | 0.005 ± 0.001 | 1 | (27) |
| MWC 1080 | 1.6 | 229 | 0.308 ± 0.039 | 7 | (14) |
| LkHa 259 | 1.0 | 18 | 93.196 ± 40.276 | 1 | (10) |
References. mm flux measurements: (1) Sandell et al. (2011); (2) Mannings & Sargent (1997); (3) Guedel et al. (1989); (4) Acke et al. (2004); (5) Péricaud et al. (2017); (6) Henning et al. (1994b); (7) Hillenbrand et al. (1992); (8) Mendigutía et al. (2012); (9) Ginsburg et al. (2013); (10) Planck Collaboration (2013); (11) Sylvester et al. (1996); (12) Barenfeld et al. (2016); (13) Meeus et al. (2012); (14) Mannings (1994); (15) Di Francesco et al. (2008); (16) Mannings & Sargent (2000); (17) Pezzuto et al. (1997); (18) Kauffmann et al. (2008); (19) Kraus et al. (2017); (20) Piétu et al. (2006); (21) Piétu et al. (2003); (22) Sylvester et al. (2001); (23) Sheret et al. (2004); (24) Cotten & Song (2016); (25) Henning et al. (1993); (26) Ribas et al. (2018); (27) Natta et al. (1997); (28) Planck Collaboration Int. LIV. (2018); (29) Urquhart et al. (2014); (30) Enoch et al. (2008); (31) Boissier et al. (2011); (32) Natta et al. (2000); (33) Alonso-Albi et al. (2009); (34) Reipurth et al. (1993); (35) Giannini et al. (1996); (36) Mairs et al. (2016).
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