Open Access
Table B.1
Intensities of gas cooling lines and PAH emission in Herbig Ae/Be protoplanetary disks.
| Object Name | [OI] 63 µm | [OI] 145 µm | [CII] 158 µm | PAHs | Re |
|---|---|---|---|---|---|
| AB AUR | 851.2 | 44.60 | 51.00 | 17.9 | 0.0053 |
| HD 97048 | 1592.0 | 65.6 | 106.8 | 55.9 | 0.0029 |
| HD 100453 | 66.10 | - | - | 7.10 | 0.0009 |
| HD 100546 | 6043.0 | 194.7 | 203.8 | 92.2 | 0.0070 |
| HD 135344 | 47.90 | - | - | 1.09 | 0.0044 |
| HD 141569 | 245.3 | 24.90 | 11.40 | 2.60 | 0.0108 |
| HD 139614 | 44.50 | - | - | 10.4 | 0.0004 |
| HD 142527 | 53.80 | - | - | 2.80 | 0.0019 |
| HD 163296 | 208.4 | - | - | 4.10 | 0.0051 |
| HD 169142 | 91.50 | - | - | 10.16 | 0.0009 |
Notes. Intensities for cooling lines are in 10−18Wm−2 (from Meeus et al. 2012) and for PAHs in 10−14 Wm−2 (from Acke & van den Ancker 2004). Re values are calculated using Eq. 2.
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