Table C.1
Observed and modeled free-free radio fluxes (top) and dustcontinuum FIR fluxes (bottom).
| ν [GHz] |
Date | Fν,radio [µJy] a | ||
|---|---|---|---|---|
| VLA | model A | model B | ||
| 8.41 | 05/95 | 385 ± 60 | 416 | 541 |
| 8.44 | 12/89 | 250 | 418 | 544 |
| 14.94 | 12/89 | 800 | 1183 | 1537 |
| λ [µm] | Fν,FIR [Jy] b | |||
| [GHz] | observed | model A | model B | |
| 24.5 | 656 | 737 | 1615 | |
| 25.3 | 554 ± 33 | 679 | 1534 | |
| 37.1 | 294 ± 18 | 101 | 620 | |
| 70.0 | 46.8 ± 8.4 | 28.9 | 105 | |
Notes. (a)The 05/95 measurement is from a visibility fit to VLA archive data, those in 12/89 are from Wendker (1995, sequential numerical identification 3502). (b)The observed fluxes (with uncertainties where provided) are from: de Wit et al. (2008, Subaru 24.5 µm), Shenoy et al. (2016, SOFIA/FORCAST 25.3 and 37.1 µm), Maercker et al. (2022, PACS 70 µm). The latter includes contributions from the outer CSE and interaction with the ISM.
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