Table 6
Maser/maser and maser/8 μm IR continuum flux ratios
| Object | F43 GHz/F86 GHz | F86 GHz/F8 μm | Ref. 43 GHz |
|
|
|||
| FMR2006 1 | 0.76 | ... | (1) |
| FMR2006 3 | ... | ... | |
| FMR2006 4 | 0.89 | ... | (1) |
| FMR2006 13 | 0.89 | 0.18 | (1) |
| X 18 | 0.95 | 0.90 | (1) |
| Stephenson 2 DFK 2 | 1.26 | 0.08 | (2) |
| Stephenson 2 DFK 49 | 0.95 | 0.82 | (2) |
| Stephenson 2 DFK 1 | 0.35 | 0.10 | (2) |
| NGC 7419/MY Cep | 1.38 | 0.09 | (3) |
| W Per | 0.41 | ... | (4) |
| S Per | 0.21 | ... | (5) |
| MDI2009 GLIMPSE13 1 | 0.41 | 0.07 | (2) |
| Cl Trumpler 27 1 | 0.16 | 0.33 | (6) |
| IK Tau (Mira) | 1.22 | ... | (7) |
| U Her (Mira) | 0.37 | ... | (7) |
Notes. Columns are (from left to right) designations of the targeted RSGs ratios of SiO(43 GHz peak flux)/SiO(86 GHz peak flux) ratio and SiO(86 GHz peak flux)/IR(8 μm flux) (see Alcolea et al. 1990). The 8 μm fluxes are taken from the MSX and GLIMPSE catalogs. Sources without measurements were not included in these surveys, or saturated in GLIMPSE.
References. (1) Nakashima & Deguchi (2006); (2) Deguchi et al. (2010); (3) Nakashima & Deguchi (2007); (4) Jiang et al. (1996); (5) Cho et al. (1996); (6) Hall et al. (1990); (7) Kim et al. (2010).
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