Table 1
Stellar and disk parameters of the Herbig stars in our sample.
| Target | F30/F13.5 | Group | Gap? | LPAH/L∗ | I6.2/I11.3 | L ∗ | T ∗ | d | F 1300 |
| ▿ | L ⊙ | K | pc | mJy | |||||
|
|
|||||||||
| HD 35929 | 0.43 ± 0.01 | IIa | ... | ... | ... | 131.2 | 6870 | 510 | ... |
| HD 72106S | 0.49 ± 0.01 | IIa | ... | 2.48 ± 0.03 × 10-3 | 1.72 ± 0.08 | 270.9 | 10 750 | 277 | ... |
| HD 58647 | 0.49 ± 0.01 | IIa | ... | 8.30 ± 0.20 × 10-5 | ... | 270.9 | 10 750 | 277 | ... |
| HD 190073 | 0.75 ± 0.02 | IIa | ... | ... | ... | 61.9 | 8990 | 290 | ... |
| HD 98922 | 0.75 ± 0.03 | IIa | ... | ... | ... | 855.7 | 10 500 | 538 | ... |
| Wray1484 | 0.76 ± 0.02 | Ia | ... | ... | ... | 1339.9 | 30 000 | 750 | ... |
| HD 95881 | 0.77 ± 0.05 | IIa | ... | 5.52 ± 0.04 × 10-3 | 1.88 ± 0.04 | 7.7 | 8990 | 118 | ... |
| NX Pup | 0.78 ± 0.02 | IIa | ... | ... | ... | 19.6 | 7290 | 450 | ... |
| HD 50138 | 0.78 ± 0.04 | IIa | ... | ... | ... | 423.5 | 12 230 | 289 | ... |
| VV Ser | 0.79 ± 0.02 | IIa | ... | 4.11 ± 0.06 × 10-3 | 2.92 ± 0.35 | 19.1 | 9000 | 330 | ... |
| HD 85567 | 0.82 ± 0.04 | IIa | ... | 8.80 ± 0.10 × 10-4 | 1.87 ± 0.10 | 328.3 | 12 450 | 480 | ... |
| HD 37806 | 0.85 ± 0.07 | IIa | ... | 1.90 ± 0.40 × 10-3 | ... | 145.3 | 9480 | 470 | ... |
| BF Ori | 0.87 ± 0.03 | IIa | ... | 1.71 ± 0.07 × 10-4 | ... | 34.1 | 8985 | 510 | ... |
| HD 101412 | 0.92 ± 0.03 | IIa | ... | 1.90 ± 0.07 × 10-3 | 1.99 ± 0.10 | 5.1 | 9960 | 118 | ... |
| HD 144668 | 0.96 ± 0.02 | IIa | ... | ... | ... | 87.5 | 7930 | 208 | 20 ± 16o |
| KK Oph | 1.04 ± 0.02 | IIa | ... | ... | ... | 0.74 | 8030 | 145 | 52 ± 15o |
| HD 37258 | 1.10 ± 0.03 | IIa | ... | ... | ... | 36.2 | 8970 | 510 | ... |
| HD 31648 | 1.19 ± 0.03 | IIa | ... | 2.50 ± 0.50 × 10-3 | ... | 13.7 | 8720 | 131 | 250 ± 15r,† |
| HD 104237 | 1.28 ± 0.03 | IIa | ... | ... | ... | 34.7 | 8405 | 116 | 92 ± 19o |
| HD 150193 | 1.42 ± 0.05 | IIa | ... | ... | ... | 24.0 | 8990 | 150 | 45 ± 12r,† |
| HD 244604 | 1.43 ± 0.03 | IIa | ... | 1.30 ± 0.30 × 10-3 | ... | 23.6 | 8730 | 340 | ... |
| HD 142666 | 1.53 ± 0.05 | IIa | √ a | 1.94 ± 0.30 × 10-3 | 1.74 ± 0.09 | 14.4 | 7580 | 145 | 127 ± 9m |
| WW Vul | 1.60 ± 0.04 | IIa | ... | 3.47 ± 0.07 × 10-4 | ... | 15.8 | 8430 | 440 | ... |
| RR Tau | 1.72 ± 0.04 | IIa | ... | 2.10 ± 0.01 × 10-2 | 1.40 ± 0.02 | 2.2 | 8460 | 160 | ... |
| HD 144432 | 1.82 ± 0.06 | IIa | √ b | 2.92 ± 0.10 × 10-4 | ... | 10.1 | 7345 | 145 | 44 ± 10p |
| HD 37357 | 1.85 ± 0.04 | IIa | ... | 9.00 ± 1.00 × 10-4 | ... | 85.1 | 9230 | 510 | ... |
| HD 163296 | 2.00 ± 0.10 | IIa | ... | ... | ... | 23.3 | 8720 | 122 | 743 ± 15o |
| HD 145263 | 2.00 ± 0.10 | IIa | ... | ... | ... | 3.8 | 7200 | 116 | ... |
| HD 35187 | 2.10 ± 0.10 | IIa | ... | 1.23 ± 0.01 × 10-3 | 3.11± 0.23 | 27.4 | 8970 | 150 | 20 ± 2t |
| HD 203024 | 2.30 ± 0.20 | Ia | ... | ... | ... | 99.2 | 8200 | 620 | ... |
| HD 179218 | 2.40 ± 0.20 | Ia | ... | ... | ... | 79.2 | 9810 | 244 | 71 ± 7s |
| HD 250550 | 2.50 ± 0.10 | Ia | ... | 1.30 ± 0.10 × 10-3 | ... | 20.9 | 10 700 | 280 | ... |
| HD 259431 | 2.55 ± 0.05 | Ia | ... | ... | ... | 8294.5 | 25 400 | 800 | ... |
| HD 38120 | 2.60 ± 0.20 | Ia | ... | 1.30 ± 0.30 × 10-3 | ... | 89.3 | 10 500 | 510 | ... |
| HD 100546 | 3.50 ± 0.20 | Ia | √ c | ... | ... | 32.9 | 10 500 | 103 | 465 ± 20o |
| HD 37411 | 4.00 ± 0.20 | Ia | ... | 3.40 ± 0.10 × 10-3 | 3.62 ± 0.39 | 34.4 | 9100 | 510 | 5 ± 3o |
| HD 36112 | 4.10 ± 0.20 | Ia | √ d | 1.30 ± 0.20 × 10-3 | ... | 22.2 | 7850 | 205 | 72 ± 13s |
| HD 139614 | 4.20 ± 0.30 | Ia | √ e | 2.54 ± 0.04 × 10-3 | ... | 8.6 | 7850 | 140 | 242 ± 15m |
| AB Aur | 4.50 ± 0.10 | Ia | √ f | 4.40 ± 0.20 × 10-3 | 4.32 ± 1.18 | 46.2 | 9520 | 144 | 136 ± 15r |
| HD 142527 | 5.00 ± 0.10 | Ia | √ g | 2.95 ± 0.05 × 10-3 | 1.34 ± 0.07 | 50.6 | 6260 | 198 | 1190 ± 33p |
| T CrA | 5.00 ± 0.30 | Ia | ... | ... | ... | 0.4 | 7200 | 130 | 219 ± 11o |
| HD 100453 | 5.20 ± 0.30 | Ib | √ h | 4.70 ± 0.10 × 10-3 | 2.25 ± 0.10 | 8.0 | 7390 | 112 | 200 ± 21 q,† |
| HD 97048 | 5.90 ± 0.40 | Ib | √ i | 9.01 ± 0.03 × 10-3 | 0.87 ± 0.01 | 40.7 | 10 010 | 158 | 452 ± 34o |
| HD 141569 | 6.80 ± 0.20 | Ib | √ j | 3.53 ± 0.02 × 10-4 | 6.31 ± 0.24 | 18.3 | 9520 | 99 | 5 ± 1u |
| HD 169142 | 7.80 ± 0.50 | Ib | √ k | 6.05 ± 0.02 × 10-3 | 1.24 ± 0.01 | 15.3 | 8200 | 145 | 197 ± 15m |
| HD 34282 | 10.00 ± 0.60 | Ib | √ h | 1.55 ± 0.01 × 10-2 | 1.82 ± 0.02 | 3.1 | 8720 | 164 | 100 ± 23t |
| Oph IRS 48 | 10.40 ± 0.30 | Ib | √ l | 2.64 ± 0.02 × 10-2 | 2.94 ± 0.01 | 14.3 | 10 000 | 120 | 60 ± 10n |
| HD 135344B | 10.90 ± 0.30 | Ib | √ i | 1.80 ± 0.02 × 10-3 | 1.42 ± 0.08 | 8.3 | 6590 | 140 | 142 ± 19m |
Notes. The targets are sorted by the F30/F13.5 MIR spectral index which naturally splits most of the flat disks (group IIa) from the flaring/transitional disks (groups Ia and Ib). The PAH characteristics and the stellar parameters are adopted from Acke et al. (2010). Complementary mm photometry is taken from the literature. The † indicates that the 1.3 mm flux is extrapolated from other (sub-)mm values using the spectral slope between the FIR and the (sub-)mm fluxes.
Reference. a) Schegerer et al. (2013); b) Chen et al. (2012); c) Bouwman et al. (2003); d) Isella et al. (2010); e) Matter et al. (2014); f) Piétu et al. (2005); g) Fukagawa et al. (2006); h) Khalafinejad et al., in prep. i) Maaskant et al. (2013); j) Augereau et al. (1999); k) Honda et al. (2012); l) Geers et al. (2007a); m) Sylvester et al. (1996); n) Andrews & Williams (2007); o) Henning et al. (1994); p) Walker & Butner (1995); q) Meeus et al. (2002); r) Sandell et al. (2011); s) Mannings & Sargent (2000); t) Natta et al. (2004); u) Sylvester et al. (2001).
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