Table B.1
Template W-R and Of/WN star models. Input spectra were both flux calibrated (bold) and non-flux calibrated.
| Star | Spectral | Spectra | (mV)/mv | (AV)/Av | (MV)/Mv | T ∗ | T eff | (BCV)/BCv | log L | ν∞ | Ṁ | Abundance | L EUV | log q0 | log Q0 | Ref. | |
| BAT99 | Alias | Type | [mag] | [mag] | [mag] | [kK] | [kK] | [mag] | [L⊙] | [km s-1] | [M⊙ yr-1] | (by mass) | [LBol ] | [ph cm-2 s-1] | [ph s-1] | ||
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| 12 | Sk -67° 22 | O2 If*/WN 5 | a, b | (13.49) | (0.4) | (− 5.4) | 49.8 | 49.3 | (− 4.4) | 5.83 | 2650 | 3.7 × 10-6 | 60:39:0.3 | 0.64 | 24.79 | 49.67 | (1)+(2) |
| 97 | Mk 51 | O3.5 If*/WN 7 | c | (13.74) | (2.2) | (− 6.9) | 41.0 | 40.8 | (− 3.7) | 6.14 | 1500 | 4.7 × 10-6 | 60:39:0.5 | 0.49 | 24.40 | 49.83 | (1) |
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| 86 | Brey 69 | WN 3(h) | c | 16.68 | 1.98 | −3.75 | 79.3 | 74.9 | −5.2 | 5.43 | 1750 | 3.2 × 10-5 | 20:79:0.5 | 0.85 | 25.63 | 49.34 | (1) |
| 106 | R136a3 | WN 5h | d, e, f | 13.02 | 1.86 | −7.29 | 53.0 | 53.0 | −4.5 | 6.58 | 2200 | 3.7 × 10-5 | 40:59:0.4 | 0.69 | 24.90 | 50.47 | (3) |
| 118 | Brey 89 | WN 6h⋆ | g, h, i | 11.20 | 0.58 | −7.83 | 45.0 | 39.4 | −3.5 | 6.41 | 1450 | 8.0 × 10-5 | 20:79:0.5 | 0.54 | 24.62 | 50.26 | (1) |
| 89 | Brey 71 | WN 7h | g, c | 14.13 | 1.53 | −5.85 | 49.8 | 44.5 | −3.6 | 5.75 | 1000 | 1.9 × 10-5 | 15:84:0.5 | 0.58 | 24.96 | 49.61 | (1) |
| 96 | Brey 81 | WN 8(h) | h, c | 13.82 | 2.40 | −7.03 | 42.5 | 36.9 | −3.4 | 6.04 | 850 | 4.0 × 10-5 | 6:93:0.3 | 0.48 | 24.49 | 49.82 | (1) |
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| 88 | Brey 70a | WN 4b/WCE | c, g | 17.75 | 4.04 | −4.74 | 80.0 | 72.1 | −5.0 | 5.78 | 1750 | 1.5 × 10-5 | 99:0.5:0.1 | 0.82 | 25.66 | 49.67 | (1) |
| 90 | Brey 74 | WC 4 | e, j | 15.41 | 1.48 | −4.52 | 85.0 | 72.0 | −4.7 | 5.57 | 2600 | 1.6 × 10-5 | 45:43:11 | 0.72 | 25.76 | 49.31 | (4) |
Notes.
Values in parentheses are given in broad band and apply to Of/WN stars. Narrow band is used for all other W-R stars. All properties except for (mV)/mv are model derived. Abundance ratios are given in H:He:N for Of/WN and WN stars, He:C:N for WN/C stars and He:C:O for WC stars. See Figs. B.1–B.9 for model fits.
Recently revealed as a WN 5-6+WN 6-7 binary system by Sana et al. (2013b) but for our template model we adopt properties in the case of a single star.
Spectra: a – Hubble Space Telescope – Space Telescope Imaging Spectrograph (HST-STIS); b – Very Large Telescope – Fibre Large Array Multi-Element Spectrograph – Ultraviolet and Visual Echelle Spectrograph (VLT-FLAMES-UVES); c – VLT – FLAMES – Multi-object spectrometry mode (VLT-FLAMES-MEDUSA); d – HST-Goddard High-Resolution Spectrograph (HST-GHRS); e – HST-Faint Object Spectrograph (HST-FOS); f – VLT – Spectrograph for Integral Field Observations in the Near Infrared (VLT-SINFONI); g – Anglo Australian Telescope – Royal Greenwich Observatory Spectrograph (AAT-RGO); h – Mount Stromlo Observatory Coudé Spectrograph (MSO); i – International Ultraviolet Explorer (IUE-HIRES); j – Siding Spring Telescope – Dual-Beam Spectrograph (SSO-DBS).
Reference. (1) This work; (2) Doran & Crowther (2011); (3) Crowther et al. (2010); (4) Crowther et al. (2002).
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