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Table 5:

Line fluxes of the PAHs features at 8.6 $\mu $m and line fluxes of the PAHs complex at 11 $\mu $m.

Star
PAHs 8.6 (W/m2)   Comp 11 (W/m2)   Ref.
HD 142527 <9.90 $\times$ 10-15   2.09 $\times$ 10-14   1
HD 169142 2.55 $\times$ 10-14   8.18 $\times$ 10-15   1
HD 150193A <3.64 $\times$ 10-15   8.29 $\times$ 10-15   1
HD 163296 <5.57 $\times$ 10-15   1.49 $\times$ 10-14   1
HD 100546 5.61 $\times$ 10-14   3.89 $\times$ 10-13   1
HD 98922 y   1.4 $\times$ 10-14   2, 3
HD 250550 n   n   4
HD 259431 -   -   -
HD 45677 -   -   -
UX Ori <1.57 $\times$ 10-15   <7.20 $\times$ 10-16   1
HD 100453 <1.65 $\times$ 10-14   7.83 $\times$ 10-15   1
HD 101412 y   1.5 $\times$ 10-15   2, 3
HD 104237 <2.67 $\times$ 10-15   <1.56 $\times$ 10-15   1
HD 142666 <5.37 $\times$ 10-15   5.42 $\times$ 10-15   1
49 Cet -   -   -
MWC 758 -   -   -
V892 Tau -   -   -
VV Ser <1.67 $\times$ 10-15   2.04 $\times$ 10-15   1
HD 97048 4.52 $\times$ 10-14   3.97 $\times$ 10-14   1
AB Aur 3.68 $\times$ 10-14   4.61 $\times$ 10-14   1

Notes.  - Data not available. ``Y'' (yes): presence of PAHs features but flux not measured, ``N'' (no): absence of PAHs features.

References. References: 1: Acke & van den Ancker (2004); 2: Geers et al. (2006); 3: Geers et al. (2007); 4: Habart et al. (2004);


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