Table 2
Observed fluxes, extinctions, and effective temperatures derived using the equation of Furness et al. (2010).
| Source | F ArIII | F NeII | AV(low)a | T (low) | AV(high) | T(high) | SpT | |
| (erg s-1 cm-2) | (erg s-1 cm-2) | mag | 103 K | mag | 103 K | adoptedb | ||
|
|
||||||||
| RCW106-MMS5 IRS1 | 2.6E-11 | 1.8E-10 | 16 | 41 ± 7 | 119 | 59 ± 8 | O5 | |
| RCW106-MMS5 IRS2 | 2.5E-11 | 9.6E-11 | 16 | 44 ± 7 | 119 | 62 ± 9 | O4 | |
| RCW106-MMS68 | 2.1E-12 | 1.3E-11 | 13 | 26 ± 10 | 108 | 43 ± 7 | O9 | |
| RCW122_1 | 5.9E-14 | 3.4E-12 | 20 | 29 ± 10 | 79 | 40 ± 8 | O8.5 | |
| RCW122_2 | ... | 7.1E-13 | ... | ... | ... | ... | ... | |
Notes. The assumed uncertainty for the fluxes listed was 30%.
Extinction estimates used for RCW106-MMS5, RCWMMS-68, and RCW122 are from Fujiyoshi et al. (2006), Bik et al. (2006), and Arnal et al. (2008) respectively.
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