Table 6.
Mass-loss rate determinations of WRs.
| Source | Spectral type | ATCA  (M⊙ yr−1) |
||
|---|---|---|---|---|
| All | 5.5 GHz | 9 GHz | ||
| WR A | WN7b+OB? | 7.02 ± 0.35e−05 | – | 4.01 ± 2.50e−05 |
| WR D | WN7o | 5.92 ± 0.31e−05 | 2.97 ± 0.74e−05 | 3.09 ± 0.41e−05 |
| WR G | WN7o | 3.41 ± 0.30e−05 | – | – |
| WR I | WN8o | 3.10 ± 0.11e−05 | 1.62 ± 0.32e−05 | 2.96 ± 0.15e−05 |
| WR L | WN9h+OB? | 2.72 ± 0.15e−05 | 1.55 ± 0.32e−05 | 2.35 ± 0.16e−05 |
| WR S | WN10−11h/BHG | 0.63 ± 0.12e−05 | – | 0.34±0.10e−05 |
| WR E | WC9 | 3.62 ± 0.42e−05 | – | 2.90 ± 0.40e−05 |
| WR F | WC9d+OB? | 6.62 ± 0.34e−05 | 3.62 ± 0.74e−05 | 6.76 ± 0.44e−05 |
| WR M | WC9d | 5.74 ± 0.71e−05 | – | 3.84 ± 0.72e−05 |
Notes. Mass-loss rates are calculated from fluxes given by the FULLCONCAT, FULL5 and FULL9 datasets. These mass-loss rates are calculated for objects where an approximation of a thermally emitting stellar wind is considered valid, using the Wright and Barlow equation (Wright & Barlow 1975).
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