Table 5
Results for the fit of the synthetic SED to the IRS data using the HST shape model.
η | I | Rotation | Cross-section | γ (IRS) | Tdust | ![]() |
![]() |
γ (MIPS) |
---|---|---|---|---|---|---|---|---|
[J K−1 m−2 s−1∕2] | [K] | [106 m2] | [106 m2] | |||||
0.7 | 0 | N/A | min | 1.31 | 262 | 24 | 75 | 0.83 |
max | 0.64 | 267 | 29 | 79 | ||||
0.7 | 50 | Prograde | min | 1.61 | 254 | 13 | 64 | 0.89 |
max | 0.75 | 264 | 25 | 75 | ||||
Retrograde | min | 2.25 | 267 | 14 | 57 | 0.97 | ||
max | 0.95 | 265 | 24 | 73 | ||||
0.7 | 100 | Prograde | min | 1.79 | 248 | 7 | 60 | 0.97 |
max | 0.90 | 258 | 21 | 73 | ||||
Retrograde | min | 3.42 | 270 | 0 | 34 | 1.07 | ||
max | 1.37 | 262 | 16 | 63 | ||||
0.7 | 200 | Prograde | min | 2.12 | 242 | 0 | 53 | 1.09 |
max | 1.21 | 249 | 12 | 67 | ||||
Retrograde | min | 0.47 | 302 | 31 | 70 | 1.21 | ||
max | 2.21 | 251 | 0 | 44 | ||||
0.8 | 0 | N/A | min | 1.85 | 255 | 17 | 69 | 0.90 |
max | 0.95 | 259 | 23 | 75 | ||||
0.8 | 50 | Prograde | min | 2.21 | 246 | 2 | 54 | 0.97 |
max | 1.09 | 255 | 18 | 70 | ||||
Retrograde | min | 3.22 | 262 | 3 | 44 | 1.06 | ||
max | 1.33 | 260 | 17 | 66 | ||||
0.9 | 0 | N/A | min | 2.51 | 247 | 7 | 61 | 0.97 |
max | 1.28 | 253 | 16 | 69 | ||||
1.0 | 0 | N/A | min | 3.08 | 242 | 0 | 54 | 1.04 |
max | 1.67 | 245 | 7 | 63 |
Notes. Combinations (η, I) in bold are compatible with both IRS and MIPS observations. Rotation defines the sense of rotation (P for prograde, R for retrograde, N/A for a null thermalinertia). Cross-section is the cross-section facing SST at the time of observation: minimum or maximum (see text for details). γ (IRS) is the derived scaling factor for the IRS infrared flux. Tdust is the derived temperature of the dust. is the derived dust cross-section in the SL field of view.
is the derived dust cross-section in the LL field of view. γ (MIPS) is the scaling factor for the MIPS infrared flux from Table 4.
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