Table 1
Coordinates and spectral types of the Herbig stars used in this work and the calculated Band 6 and 7 flux densities and dust masses of each Herbig disk.
| Name | RAJ2000 | DecJ2000 | Sp.Tp. | Group | Fcont. | Mdust | Rdust, 68% | Rdust, 90% | inc | PA | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (h:m:s) | (deg:m:s) | (mJy) | (M⊕) | (au) | (au) | (°) | (°) | ||||
| AB Aurα | 04:55:45.9 | +30:33:04 | A0 | I | 192.8 | 11.8 ± 1.2 | 186 ± 15 | 225 ± 34 | 23.2 | 99 | 1, i, β |
| AK Sco | 16:54:44.9 | –36:53:19 | F5 | II | 26.1 | 6.1 ± 0.6 | 42 ± 3 | 53 ± 15 | 71 | 39 | 2, ii, β |
| BF Ori | 05:37:13.3 | –06:35:01 | A7 | II | 0.8 | 1.1 ± 0.1 | <233 | <311 | – | – | 3, β |
| CQ Tauα | 05:35:58.5 | +24:44:54 | F5 | I | 144.0 | 44.2 ± 4.8 | 62 ± 4 | 76 ± 18 | 35 | 35 | 4, iii, β |
| HD 100453 | 11:33:05.6 | –54:19:29 | A9 | I | 141.1 | 17.5 ± 1.8 | 39 ± 2 | 44 ± 6 | 38 | 128 | 5, iv, β |
| HD 100546 | 11:33:25.4 | –70:11:41 | A0 | I | 399.6 | 38.0 ± 3.9 | 35 ± 2 | 41 ± 4 | 43 | 131 | 6, v, β |
| HD 104237α | 12:00:05.1 | –78:11:35 | A0 | II | 88.9 | 10.5 ± 1.1 | <59 | <98 | – | – | 5, β |
| HD 135344B | 15:15:48.5 | –37:09:16 | F8 | I | 539.7 | 35.2 ± 3.8 | 81 ± 10 | 109 ± 31 | 11 | 28 | 7,vi, β |
| HD 139614 | 15:40:46.4 | –42:29:54 | A9 | I | 197.2 | 41.7 ± 4.3 | <65 | <97 | – | – | 6, β |
| HD 141569 | 15:49:57.8 | –03:55:16 | A2 | II | 3.4 | 0.36 ± 0.04 | <139 | <232 | – | – | 6, β |
| HD 142527 | 15:56:41.9 | –42:19:23 | F6 | I | 1048.1 | 214.9 ± 22.1 | 208 ± 9 | 236 ± 33 | 27 | 71 | 8, vii, β |
| HD 142666 | 15:56:40.0 | –22:01:40 | F0 | II | 118.6 | 25.1 ± 2.6 | 40 ± 3 | 52 ± 11 | 60 | 109 | 6, viii, β |
| HD 163296 | 17:56:21.3 | –21:57:22 | A1 | II | 541.3 | 46.7 ± 5.0 | 71 ± 6 | 101 ± 16 | 45 | 137 | 4, ix, β |
| HD 169142α | 18:24:29.8 | –29:46:49 | F1 | I | 203.7 | 22.9 ± 2.4 | 71 ± 7 | 140 ± 77 | 13 | 5 | 6, x, β |
| HD 176386α | 19:01:38.9 | –36:53:27 | B9 | II | <0.32 | <0.06 | – | – | – | – | 9, γ |
| HD 245185 | 05:35:09.6 | +10:01:52 | A0 | I | 34.6 | 41.5 ± 7.6 | <76 | <126 | – | – | 10, β |
| HD 290764 | 05:38:05.3 | –01:15:22 | F0 | I | 210.1 | 90.3 ± 11.8 | 119 ± 16 | 167 ± 28 | 30 | 154.6 | 5, xi, β |
| HD 31648α | 04:58:46.3 | +29:50:37 | A5 | II | 253.0 | 70.9 ± 7.7 | 58 ± 18 | 107 ± 49 | 37 | 122 | 4, xii, β |
| HD 34282 | 05:16:00.5 | –09:48:35 | B9.5 | I | 99.0 | 86.8 ± 9.7 | 189 ± 18 | 260 ± 77 | 60 | 150 | 11, xiii, β |
| HD 36112α | 05:30:27.5 | +25:19:57 | A8 | I | 70.7 | 18.8 ± 2.0 | 90 ± 17 | 123 ± 50 | 21 | 65 | 5, xiv, β |
| HD 37258α | 05:36:59.3 | –06:09:16 | A3 | II | 1.8 | 2.4 ± 0.4 | <326 | <435 | – | – | 3, β |
| HD 53367α | 07:04:25.5 | –10:27:16 | B0 | ? | <0.81 | <0.05 | – | – | – | – | 12 |
| HD 58647α | 07:25:56.1 | –14:10:44 | B9 | II | 1.9 | 1.0 ± 0.1 | <75 | <126 | – | – | 13, β |
| HD 9672α | 01:34:37.9 | –15:40:35 | A1 | II | 4.1 | 0.13 ± 0.01 | 315 ± 39 | 473 ± 111 | 81 | 161 | 13, xv, β |
| HD 97048 | 11:08:03.3 | –77:39:18 | A0 | I | 711.4 | 155.9 ± 16.0 | 182 ± 19 | 245 ± 69 | 41 | 85 | 14, xvi, β |
| HR 5999 | 16:08:34.3 | –39:06:18 | A7 | II | 26.5 | 4.0 ± 0.4 | <48 | <81 | – | – | 15, β |
| KK Ophα | 17:10:08.1 | –27:15:19 | A6 | II | 27.7 | 17.4 ± 2.5 | <88 | <88 | – | – | 16, δ |
| MWC 297 | 18:27:39.5 | -03:49:52 | B1.5 | I | 288.7 | 65.7 ± 9.6 | <169 | <253 | – | – | 17, β |
| R CrAα | 19:01:53.7 | –36:57:09 | B5 | II | 561.4 | 112.6 ± 27.9 | <328 | <492 | – | – | 18, ϵ |
| TY CrAα | 19:01:40.8 | –36:52:34 | B9 | I | 0.67 | 0.10 ± 0.01 | <27 | <34 | – | – | 5, β |
| V1787 Oriα | 05:38:09.3 | -06:49:17 | A5 | I | 14.8 | 24.2 ± 2.9 | <313 | <391 | – | – | 5, β |
| V599 Ori | 05:38:58.6 | –07:16:46 | A8.9 | I | 55.9 | 75.0 ± 8.6 | <328 | <410 | – | – | 19, β |
| V718 Sco | 16:13:11.6 | –22:29:07 | A5 | II | 49.5 | 11.9 ± 1.3 | <69 | <114 | – | – | 20, β |
| V892 Tauα | 04:18:40.6 | +28:19:15 | A0 | I | 285.4 | 76.1 ± 8.3 | 40 ± 4 | 52 ± 13 | 54.5 | 52.1 | 21, xvii, ζ |
| VV Ser | 18:28:47.9 | +00:08:40 | B5 | II | 2.3 | 2.3 ± 0.3 | <239 | <399 | – | – | 22, β |
| Z CMaα | 07:03:43.2 | –11:33:06 | B5 | I | 29.3 | 7.6 ± 6.4 | <28 | <41 | – | – | 23, β |
Notes. All distances are obtained from Vioque et al. (2018). The luminosities, stellar masses, and ages were obtained from Wichittanakom et al. (2020) except the objects marked with an α of which these parameters were obtained from Vioque et al. (2018). The objects in italics are from the Vioque et al. (2018) low-quality parallax sample, and the others are from the high-quality sample. The error on the continuum flux is 10% of the given value.
References. Spectral type references: (1) Mooley et al. (2013), (2) Houk (1982), (3) Tisserand et al. (2013), (4) Mora et al. (2001), (5) Vieira et al. (2003), (6) Gray et al. (2017), (7) Coulson & Walther (1995), (8) Houk (1978), (9) Torres et al. (2006), (10) Gray & Corbally (1998), (11) Houk & Swift (1999), (12) Tjin A Djie et al. (2001), (13) Houk & Smith-Moore (1988), (14) Irvine & Houk (1977), (15) Bessell & Eggen (1972), (16) Carmona et al. (2007), (17) Drew et al. (1997), (18) Gray et al. (2006), (19) Hsu et al. (2013), (20) Carmona et al. (2010), (21) Skiff (2014), (22) Guzmán-Díaz et al. (2021), (23) Covino et al. (1984). Inclination and position angle references: (i) Tang et al. (2017), (ii) Czekala et al. (2015), (iii) Ubeira Gabellini et al. (2019), (iv) Benisty et al. (2017), (v) Pineda et al. (2019), (vi) Stolker et al. (2016), (vii) Kataoka et al. (2016), (viii) Rubinstein et al. (2018), (ix) de Gregorio-Monsalvo et al. (2013), (x) Fedele et al. (2017), (xi) Kraus et al. (2017), (xii) Liu et al. (2019), (xiii) van der Plas et al. (2017a), (xiv) Isella et al. (2010), (xv) Hughes et al. (2017), (xvi) van der Plas et al. (2017b), (xvii) Long et al. (2021). Meeus group references: (β) Guzmán-Díaz et al. (2021), (γ) Boersma et al. (2009), (δ) Juhász et al. (2010), (ϵ) Acke & van den Ancker (2004), (ζ) Menu et al. (2015).
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