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Table B.5
Integrated line strengths Iint (W m-2) for additional emission lines in the PACS spectra of OT2 carbon stars observed in the new observation setting, which cannot be attributed to CO or H2O and remain unidentified.
V384 Per | R Lep | W Ori | S Aur | U Hya | Y CVn | AFGL 4202 | ||
|
||||||||
PACS | λ 0 | I int | ||||||
band | μm | (W m-2) | ||||||
|
||||||||
R1B | 180.7 | 1.95e-17 (25.73%) | ⋆ 2.18e-17 (25.71%) | ⋆ 5.95e-18 (35.55%) | / | / | / | ⋆ 2.08e-17 (27.59%) |
174.4 | / | / | / | / | / | / | 6.57e-18 (49.27%) | |
173.9 | 1.24e-17 (38.63%) | 1.47e-17 (37.82%) | 7.40e-18 (43.41%) | / | 7.59e-18 (33.54%) | 3.52e-17 (22.46%) | ⋆ 1.76e-17 (32.39%) | |
173.4 | / | / | / | 9.52e-18 (34.03%) | / | / | / | |
R1A | 145.7 | / | / | / | / | / | 8.00e-18 (29.95%) | / |
145.0 | ⋆ 1.90e-17 (25.25%) | / | ⋆ 1.98e-17 (22.86%) | ⋆ 1.10e-17 (24.37%) | / | ⋆ 5.45e-17 (20.46%) | / | |
143.5 | 1.46e-17 (23.57%) | / | / | / | / | / | / | |
143.2 | 1.46e-17 (23.50%) | 3.86e-17 (22.35%) | / | / | 6.71e-18 (26.92%) | / | / | |
139.3 | 2.06e-17 (35.10%) | 2.87e-17 (25.67%) | 1.68e-17 (21.84%) | / | 9.31e-18 (27.22%) | 5.15e-17 (20.40%) | / | |
137.9 | 1.83e-17 (27.77%) | 2.32e-17 (22.14%) | 2.51e-17 (21.50%) | ⋆ 1.30e-17 (22.55%) | / | 1.84e-17 (22.59%) | / | |
109.0 | 3.60e-17 (28.44%) | 4.11e-17 (24.23%) | / | 9.03e-18 (50.00%) | 2.19e-17 (28.87%) | ⋆ 1.18e-16 (26.50%) | / | |
108.5 | / | 1.84e-17 (31.88%) | / | 1.23e-17 (26.41%) | / | ⋆ 7.15e-17 (25.05%) | / | |
107.6 | / | / | 1.69e-17 (24.99%) | / | / | ⋆ 2.84e-17 (30.38%) | / | |
B2B | 89.5 | 5.92e-17 (22.40%) | 7.54e-17 (23.63%) | / | / | 3.88e-17 (28.88%) | ⋆ 4.45e-17 (26.32%) | / |
87.3 | ⋆ 4.99e-17 (24.99%) | ⋆ 8.31e-17 (21.38%) | 2.62e-17 (24.60%) | / | ⋆ 3.55e-17 (24.79%) | 2.73e-17 (25.43%) | 2.08e-17 (29.61%) | |
86.9 | / | 3.69e-17 (28.39%) | / | / | / | / | / | |
72.6 | 2.41e-17 (28.20%) | 6.10e-17 (25.59%) | / | 1.47e-17 (29.33%) | 1.45e-17 (34.68%) | / | / | |
72.5 | / | 4.67e-17 (27.97%) | / | / | / | / | / | |
B3A | 66.4 | / | / | / | / | / | / | ⋆ 1.66e-17 (26.53%) |
Notes. See Table B.4 for further clarification of the given information.
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