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Table 2
Best fit parameters for the Lorentz fits to the detected 69 μm bands.
Source name | # | A (Jy) | A/cont | Δp (×10) | w (×10) |
(×100) | μm | μm | |||
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OH 32.8−0.3 | 1 | 5.2 ± 0.4 | 7.2 ± 0.6 | 1.2 ± 0.2 | 2.5 ± 0.4 |
OH 21.5+0.5 | 2 | 4.4 ± 0.3 | 5.5 ± 0.4 | 1.9 ± 0.3 | 3.0 ± 0.5 |
OH 30.1−0.7 | 3 | 7.2 ± 1.0 | 4.5 ± 0.6 | 0.6 ± 0.2 | 1.8 ± 0.4 |
OH 26.5+0.6 | 4 | 13.3 ± 2.7 | 3.0 ± 0.6 | 1.1 ± 0.3 | 1.7 ± 0.8 |
OH 127.8+0.0 | 5 | 4.5 ± 0.3 | 4.6 ± 0.3 | 0.9 ± 0.3 | 3.5 ± 0.7 |
AFGL 2403 | 6 | 4.8 ± 0.4 | 5.9 ± 0.5 | 1.1 ± 0.2 | 2.9 ± 0.8 |
IRAS 21554 | 7 | 2.8 ± 0.3 | 8.2 ± 0.9 | 0.8 ± 0.1 | 1.3 ± 0.2 |
AFGL 5379 | 8 | 16.0 ± 3.8 | 2.7 ± 0.6 | 1.5 ± 0.7 | 3.6 ± 1.4 |
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RAFGL 4205 | 16 | 5.5 ± 0.9 | 3.4 ± 0.6 | 0.5 ± 0.5 | 4.7 ± 1.3 |
AFGL 6815 | 17 | 10.5 ± 0.8 | 4.9 ± 0.4 | −0.1 ± 0.2 | 3.9 ± 0.8 |
HD 161796 | 18 | 5.3 ± 1.1 | 4.3 ± 0.9 | 0.4 ± 0.2 | 2.1 ± 0.5 |
IRAS 16342 | 19 | 6.2 ± 3.2 | 1.9 ± 1.0 | −0.4 ± 0.6 | 2.0 ± 0.7 |
CPD-642939 | 20 | 5.2 ± 0.8 | 8.8 ± 1.3 | −0.2 ± 0.1 | 1.5 ± 0.3 |
OH 231.8+4.2 | 21 | 26.9 ± 4.6 | 2.6 ± 0.4 | −0.4 ± 0.6 | 2.5 ± 1.0 |
IRAS 16279 | 22 | 5.5 ± 1.5 | 4.1 ± 1.1 | −0.1 ± 0.4 | 1.2 ± 0.8 |
HDE 330036 | 23 | 1.4 ± 0.1 | 8.5 ± 0.7 | −0.6 ± 0.2 | 1.9 ± 0.3 |
IRAS 09425 | 24 | 6.2 ± 0.2 | 28.6 ± 0.9 | 0.4 ± 0.1 | 2.4 ± 0.1 |
RedRect | 28 | 7.3 ± 0.6 | 4.8 ± 0.4 | 1.1 ± 0.3 | 4.0 ± 0.8 |
ACHer | 29 | 1.4 ± 0.1 | 6.0 ± 0.4 | 1.7 ± 0.3 | 3.3 ± 0.5 |
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NGC 6543 | 34 | 9.5 ± 1.6 | 10.2 ± 1.7 | −0.2 ± 0.1 | 1.4 ± 0.2 |
NGC 6302 | 35 | 93.4 ± 16.9 | 10.3 ± 1.9 | −0.5 ± 0.1 | 1.2 ± 0.2 |
NGC 6537 | 36 | 24.1 ± 3.9 | 11.9 ± 1.9 | −0.4 ± 0.1 | 1.2 ± 0.3 |
CPD-568032 | 37 | 18.0 ± 4.4 | 9.3 ± 2.3 | −0.2 ± 0.1 | 1.4 ± 0.2 |
BD +303639 | 38 | 5.4 ± 1.6 | 4.0 ± 1.2 | 0.3 ± 0.5 | 2.0 ± 1.0 |
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AFGL 4106 | 42 | 11.2 ± 4.3 | 1.7 ± 0.7 | −0.4 ± 0.7 | 1.8 ± 1.0 |
HD 168625 | 43 | 11.1 ± 0.4 | 13.1 ± 0.5 | 1.2 ± 0.1 | 2.5 ± 0.1 |
AFGL 2343 | 44 | 16.7 ± 3.2 | 3.6 ± 0.7 | 0.6 ± 0.3 | 1.6 ± 0.4 |
Notes. Amplitude (A), wavelength shift of the peak wavelength position relative to 69.0 μm (Δp), and the width of the Lorentz curve (w).
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