Table 2
Parameters of the DWCL source candidates.
| IRAS source | l | b | C 12 | C 23 | Fir(Jy) | Lir(103 L⊙) |
|
|
||||||
| 21147+5016 | 92 05 |
097 |
−0.34 | 0.21 | 9.5 ± 0.2 | 3.0 ± 1.2 |
| 21106+5013 | 9156 |
141 |
−0.32 | 0.02 | 11.2 ± 0.2 | 4.0 ± 1.6 |
| 21093+4959 | 9125 |
139 |
−0.34 | 0.16 | 9.2 ± 0.2 | 3.3 ± 1.3 |
| 21041+5052 | 9134 |
260 |
−0.32 | −0.33 | 27.1 ± 0.2 | 9.6 ± 3.8 |
Notes. DWCL refers to a dusty late-type Wolf-Rayet star. Cij = log (Fj/Fi), where i and j run from 1 to 4 and correspond to 12, 25, 60 and 100 μm, respectively and Fi is the flux density (Jy) in band i. Lir/
, where the integrated flux in Jy is Fir = 1.3(F12 + F25) + 0.7(F25 + F60) + 0.2(F60 + F100) (Chan & Fich 1995). Subscripts are wavelengths in microns. Luminosity values are for d = 15 kpc.
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