Table 5: The continuum flux at the peak wavelength of the IR features included in this analysis. When the amorphous 10 micron silicate band was present, the PAH features are superimposed on the band. In this case (flagged by $^\ast $), the silicate feature is regarded as being part of the underlying continuum of the PAH features. Hence the indicated continuum flux of the PAH band is the flux of the silicate feature at the central wavelength of that PAH band.
CF at the peak wavelength of the IR features
Object Group PAH 3.3 NAN 3.4 NAN 3.5 PAH 6.2 PAH 7.7 PAH 8.6 COMP 11 Si 9.7
    [Jy] [Jy] [Jy] [Jy] [Jy] [Jy] [Jy] [Jy]
V376 Cas I 5.5 6.0 6.3 10.0 11.3$^\ast $ 17.1$^\ast $ 23.2$^\ast $ 13.7
Elias 3-1 I 3.1 3.3 3.5 4.0 8.0$^\ast $ 12.4$^\ast $ 32.7$^\ast $ 19.1
AB Aur I 13.1 13.1 13.0 9.1 10.0$^\ast $ 15.1$^\ast $ 24.8$^\ast $ 12.8
HD 34282 I 0.7 0.8 0.7 1.0 0.9 0.8 0.8 0.7
HD 34700 I 0.5 0.5 0.3 0.4 0.7 0.7 0.8 0.7
HD 97048 I 2.0 2.0 2.0 1.1 3.2 4.0 6.4 4.7
HD 100453 I 4.8 4.9 4.9 3.7 4.4 4.2 6.3 4.7
HD 100546 I 6.0 5.7 5.7 7.0 17.3$^\ast $ 28.8$^\ast $ 62.5$^\ast $ 28.4
HD 135344 I 3.4 3.4 3.4 2.1 1.7 1.4 1.0 1.1
HD 139614 I 1.4 1.3 1.3 1.0 1.4 1.5 2.6 2.4
HD 142527 I 6.4 6.4 6.4 7.0 7.7$^\ast $ 10.7$^\ast $ 11.9$^\ast $ 7.1
CD-42$^\circ $11721 I 23.6 25.0 25.7 41.4 44.3 43.7 45.9 39.5
HD 169142 I 1.8 1.7 1.7 1.7 1.6 1.6 2.0 1.6
T CrA I 2.2 2.2 2.3 3.0 3.3$^\ast $ 4.4$^\ast $ 8.3$^\ast $ 5.9
HD 179218 I 3.4 3.4 3.5 5.5 9.3$^\ast $ 14.2$^\ast $ 18.3$^\ast $ 10.5
BD+40$^\circ $4124 I? 5.5 5.6 5.7 7.5 9.0 9.6 8.9 8.1
HD 200775 I 11.8 11.7 11.8 9.4 9.8$^\ast $ 11.4$^\ast $ 9.3$^\ast $ 8.2
MWC 1080 I 11.2 11.6 11.7 14.5 14.9 14.6 16.2 13.6
VX Cas II 0.4 0.4 0.4 0.4 0.5$^\ast $ 0.8$^\ast $ 1.2$^\ast $ 0.7
HD 31648 II 4.0 4.0 4.0 4.6 6.1$^\ast $ 8.7$^\ast $ 11.3$^\ast $ 6.1
UX Ori II 0.9 0.9 0.9 0.8 0.9$^\ast $ 2.0$^\ast $ 2.7$^\ast $ 1.5
HD 35187 II 2.4 2.4 2.4 1.9 2.6 3.8 5.4 4.9
BF Ori II 0.4 0.4 0.4 0.5 0.6$^\ast $ 1.1$^\ast $ 1.4$^\ast $ 0.8
RR Tau II 0.9 0.9 0.9 0.9 1.1 1.2 1.6 1.3
HD 95881 II 4.0 3.9 3.9 4.5 5.5 6.9 7.8 8.0
HD 104237 II 10.8 10.8 10.8 10.8 10.6$^\ast $ 15.9$^\ast $ 22.4$^\ast $ 9.6
HD 141569 II 0.7 0.7 0.6 0.4 0.5 0.5 0.5 0.5
HD 142666 II 2.7 2.7 2.7 0.6 3.7$^\ast $ 5.5$^\ast $ 6.3$^\ast $ 2.6
HD 144432 II 2.8 2.8 2.7 2.1 2.3$^\ast $ 4.8$^\ast $ 7.4$^\ast $ 4.1
HR 5999 II 17.9 18.0 18.1 13.6 13.9$^\ast $ 15.0$^\ast $ 16.9$^\ast $ 14.7
Wra 15-1484 II 6.6 7.1 7.4 14.4 17.3 18.4 21.0 19.8
HD 150193 II 4.8 4.7 4.7 4.8 5.5$^\ast $ 13.3$^\ast $ 18.7$^\ast $ 8.8
AK Sco II 1.5 1.5 1.5 1.2 1.2$^\ast $ 1.9$^\ast $ 2.8$^\ast $ 2.0
HD 163296 II 9.8 9.7 9.6 7.2 8.8$^\ast $ 14.0$^\ast $ 20.3$^\ast $ 12.2
VV Ser II 2.5 2.5 2.5 2.6 3.1$^\ast $ 3.8$^\ast $ 4.4$^\ast $ 3.4
R CrA II? 54.2 57.0 59.2 64.6 58.3$^\ast $ 79.8$^\ast $ 126.3$^\ast $ 86.1
WW Vul II 0.9 0.9 0.8 0.7 0.8$^\ast $ 1.5$^\ast $ 2.1$^\ast $ 1.3
LkH$\alpha $ 224 II? 3.9 4.1 4.2 7.3 9.0 10.3 12.4 11.4
BD+46$^\circ $3471 II       0.6 0.9$^\ast $ 1.0$^\ast $ 1.6$^\ast $ 1.0
SV Cep II 0.6 0.7 0.7 0.8 1.1$^\ast $ 2.9$^\ast $ 4.6$^\ast $ 2.7
Z CMa III 40.1 43.3 45.2 86.9 101.7 84.3 101.9 114.7
IRAS 12496-7650 III 7.9 9.1 9.7 17.7 21.8 21.8 33.3 30.2
MWC 297 III 65.8 68.3 71.5 104.6 118.9 123.7 119.7 123.3
LkH$\alpha $ 225 III 1.3 1.5 1.7 12.6 24.5 23.8 26.2 36.8
PV Cep III 1.9 2.2 2.4 7.4 9.6 8.5 10.6 12.8
V645 Cyg III 8.3 9.6 10.7 45.2 65.7 65.4 87.5 91.0


Source LaTeX | All tables | In the text