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Table 4.
Mass-loss rates calculated using the observed flux densities at 3 mm.
| Source | Spectral type | Teff | v∞ |
|
|---|---|---|---|---|
| kK | (km s−1) | (M⊙ yr−1) | ||
| WR J | WN5h | 60 | 1500 | 1.62e−05 |
| WR R | WN5o | 60 | 1500 | 2.65e−05 |
| WR O | WN6o | 70 | 1800 | 3.92e−05 |
| WR U | WN6o | 70 | 1800 | 3.41e−05 |
| WR Q | WN6o | 70 | 1800 | 2.73e−05 |
| WR A | WN7b+OB? | 50 | 1300 | 7.19e−05 |
| WR D | WN7o | 50 | 1300 | 2.07e−05 |
| WR B | WN7o+OB? | 50 | 1300 | 3.99e−05 |
| WR G | WN7o | 50 | 1300 | 2.22e−05 |
| WR P | WN7o | 50 | 1300 | 1.92e−05 |
| WR I | WN8o | 45 | 1000 | 3.55e−05 |
| WR V | WN8o | 45 | 1000 | 2.34e−05 |
| WR L | WN9h+OB? | 32 | 700 | 3.82e−05 |
| WR S | WN10−11h | 25 | 400 | 5.18e−06 |
| W13 | WN9−10h | 28.5 | 500 | 5.52e−06 |
| WR K | WC8 | 63 | 1700 | 3.22e−05 |
| WR E | WC9 | 45 | 1200 | 5.24e−05 |
| WR F | WC9d+OB? | 45 | 1200 | 7.36e−05 |
| WR C | WC9d | 45 | 1200 | 2.74e−05 |
| WR H | WC9d | 45 | 1200 | 3.29e−05 |
| WR M | WC9d | 45 | 1200 | 3.57e−05 |
| W25 | 09Iab | 31.5 | 2100 | 8.25e−06 |
| W43a | B0Ia | 27.5 | 1500 | 5.50e−06 |
| W61a | B0.5Ia | 26.5 | 1350 | 3.65e−06 |
| W46a | B1 Ia | 22 | 725 | 3.65e−06 |
| W56a | B1.5Ia | 21 | 500 | 1.45e−06 |
| W52 | B1.5Ia | 21 | 500 | 1.50e−06 |
| W8b | B1.5Ia | 21 | 500 | 1.81e−06 |
| W28 | B2Ia | 19 | 550 | 2.57e−06 |
| W2a | B2Ia | 19 | 550 | 1.66e−06 |
| W11 | B2Ia | 19 | 550 | 1.59e−06 |
| W23a | B2Ia+BSG | 18 | 400 | 3.19e−06 |
| W71 | B2.5Ia | 19 | 550 | 2.78e−06 |
| W33 | B5Ia+ | 13 | 300 | 2.57e−06 |
| W7 | B5Ia+ | 13 | 300 | 3.64e−06 |
| W42a | B9Ia+ | 10 | 200 | 1.92e−06 |
Notes. Adopted parameters are d = 5 kpc, Z = 1, γ = 1, Twind = 0.5 × Teff. For the WR stars, μ is taken as 4.0 for WN6 or earlier, 2.0 for later than WN6, 4.7 for WC8 & WC9. See Sect. 4.2.2 for discussion of the errors.
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