Table 6
Flux levels of our VISIR imaging of the targets.
Target | PAH2 [Jy] | PAH2_2 [Jy] | SiC [Jy] | F12 [Jy] | Neb | log L12/L∗ |
|
||||||
PDS 204 | 4.2 ± 0.8 | 3.5 ± 0.7 | 3.7 ± 0.9 | 6.4 ± 0.3 | X | –7.5 ± 0.09 |
MWC 789 | 4.5 ± 0.7 | 3.8 ± 0.6 | 4.6 ± 0.7 | 4.5 ± 0.3 | X | –6.2 ± 0.06 |
LkHα 208 | 3.8 ± 0.6 | 3.0 ± 0.4 | 3.2 ± 0.5 | 3.4 ± 0.03 | X | –5.5 ± 0.06 |
LkHα 339 | 1.1 ± 0.1 | 0.9 ± 0.1 | 0.9 ± 0.1 | 6.6 ± 0.1 | X | –6.0 ± 0.05 |
MWC 137 | 3.2 ± 0.5 | 3.0 ± 0.4 | 3.1 ± 0.5 | 20.4 ± 1.0 | X | –8.1 ± 0.06 |
LkHα 215 | 0.8 ± 0.1 | 0.64 ± 0.06 | 0.7 ± 0.1 | 9.1 ± 0.5 | X | –7.6 ± 0.06 |
MWC 147 | 6.9 ± 0.1 | 5.8 ± 0.6 | 6.2 ± 0.6 | 12.8 ± 1.3 | X | –7.7 ± 0.04 |
R Mon | 41 ± 4 | 41 ± 4 | 43 ± 4 | 56.7 ± 0.1 | X | –5.1 ± 0.04 |
PDS 241 | 0.12 ± 0.05 | 0.04 ± 0.02 | 0.08 ± 0.03 | 14.1 ± 1.6 | X | –9.0 ± 0.14 |
PDS 27 | 14 ± 1 | 13.9 ± 1.4 | 15 ± 1 | 15.0 ± 0.6 | – | –6.8 ± 0.03 |
Hen 3-331 | 6.5 ± 1 | 5.8 ± 0.6 | 5.5 ± 0.8 | 6.4 ± 0.2 | – | –7.5 ± 0.06 |
Hen 3-847 | 34 ± 4 | 29 ± 2 | 30 ± 4 | 36.1 ± 1.4 | – | –5.7 ± 0.05 |
Hen 3-1110 | 0.30 ± 0.05 | 0.29 ± 0.04 | 0.31 ± 0.06 | 0.76 ± 0.1 | – | –9.2 ± 0.08 |
MCW 1264 | 0.07 ± 0.05 | 0.05 ± 0.04 | 0.08 ± 0.06 | 13.3 ± 4.2 | – | – |
V921 Sco | 35 ± 7 | 29 ± 4 | 34 ± 6 | 124.2 ± 7.5 | X | –7.6 ± 0.07 |
MWC 878 | 23 ± 5 | 20 ± 3 | 21 ± 4 | 21.1 ± 1.3 | – | –6.8 ± 0.08 |
Hen 3-1418 | 0.04 ± 0.02 | 0.03 ± 0.02 | 0.07 ± 0.02 | 2.5 ± 0.2 | – | – |
Hen 3-1444 | 6.2 ± 1.2 | 5.7 ± 0.8 | 5.5 ± 1.1 | 6.7 ± 0.4 | – | – |
PDS 152 | 0.13 ± 0.05 | 0.18 ± 0.04 | 0.12 ± 0.04 | 3.7 ± 0.4 | – | – |
MWC 593 | 0.10 ± 0.03 | 0.10 ± 0.03 | 0.09 ± 0.03 | <1.6 | – | – |
PDS 477 | 2.3 ± 0.3 | 2.1 ± 0.3 | 2.2 ± 0.3 | 2.8 ± 0.25 | – | –7.1 ± 0.06 |
LkHα 115 | 0.4 ± 0.1 | 0.29 ± 0.04 | 0.28 ± 0.06 | – | X | – |
LkHα 260 | 0.6 ± 0.1 | 0.44 ± 0.07 | 0.48 ± 0.07 | 1.0 ± 0.9 | X | –6.7 ± 0.06 |
MWC 297 | 121 ± 18 | 113 ± 17 | 123 ± 18 | 159 ± 6.3 | X | –7.4 ± 0.06 |
AS 310 | 1.4 ± 0.6 | 1.1 ± 0.5 | 1.2 ± 0.5 | 51.5 ± 0.2 | X | –7.8 ± 0.15 |
PDS 543 | 2.3 ± 0.5 | 1.9 ± 0.3 | 2.0 ± 0.4 | 4.2 ± 0.2 | – | –7.9 ± 0.08 |
Notes. The F12 column represents the 12 μm IRAS measurement (MSX C for LkHα 260). The column underneath “Neb” indicates whether an optical reflection nebula is present in the Digitized Sky Survey at 0.65 μm. In the last column we derived the 12 μm excess fraction of the circumstellar disks. For Hilt 641, AS 267, NGC 6530-45, and LkHa 112 we supply an upper limit of 0.1 Jy in the SiC filter.
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