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Table 2
Total MIR/FIR/submm flux densities of NGC 891.
Wavelength | Fν | Error (Fν) | Telescope | Reference | |
μm | Jy | Jy | |||
|
|||||
12 | 5.46 | 0.82 | IRAS | Rice et al. (1988); Sanders et al. (2003) | average |
25 | 7.39 | 1.11 | IRAS | Rice et al. (1988); Sanders et al. (2003) | average |
60 | 63.8 | 9.6 | IRAS | Rice et al. (1988); Sanders et al. (2003) | average |
100 | 185 | 28 | IRAS | Rice et al. (1988); Sanders et al. (2003) | average |
170 | 193 | 18 | ISO | Popescu et al. (2004) | – |
200 | 165 | 17 | ISO | Popescu et al. (2004) | – |
450 | 40.95 | 8.0 | SCUBA | Israel et al. (1999) | extrapolated |
850 | 4.85 | 0.6 | SCUBA | Israel et al. (1999) | extrapolated |
1200 | 0.92 | 0.13 | IRAM | Guelin et al. (1993) | extrapolated |
Notes. The observed flux densities available only within a fixed aperture were extrapolated to the whole galaxy using the best fit model of NGC 891.
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