Table 1
WR stars with spectropolarimetry from Harries et al. (1998): circumstellar, and spectropolarimetric properties of the sample stars.
| WR | Spec. type | LE | RN | NF | C iv | |||
|
|
||||||||
| 006 | WN4b | + | W, E | NF++ | 84.6 | |||
| 016 | WN8h | + | W/E | NF− | 278.8 | |||
| 040 | WN8h | + | W/E | NF++ | 287.1 | |||
| 134 | WN6b | + | W | NF+ | 113.3 | |||
| 136 | WN6 | + | W/E | NF+ | 145.2 | |||
| 137 | WC7+OB | + | − | NF+ | 110.8 | |||
|
|
||||||||
| 014 | WC7 | − | R | NF− | 67.4 | |||
| 018 | WN4b | − | W, W/E | |||||
| 024 | WN6ha | − | − | NF+ | 116.7 | |||
| 078 | WN7h | − | − | NF− | 73.2 | |||
| 104 | WC9 | − | − | |||||
| 110 | WN5-6b | − | − | |||||
| 111 | WC5 | − | − | NF− | 91.4 | |||
| 121 | WC9 | − | − | |||||
| 127 | WN3b+O9.5V | − | − | |||||
| 128 | WN4(h) | − | R | NF− | 59.5 | |||
| 133 | WN5o+O9I | − | RN?? | NF+ | 109.9 | |||
| 135 | WC8 | − | − | NF+ | 98.3 | |||
| 138 | WN5o+B? | − | − | NF+ | 98.4 | |||
| 139 | WN50+O6 | * | − | NF− | 62.8 | |||
| 141 | WN6+O5 | * | − | |||||
| 143 | WC4 | − | − | |||||
| 148 | WN8h | − | − | NF++ | − | |||
| 150 | WC5 | − | − | |||||
| 152 | WN3(h) | − | − | |||||
| 153ab | WN6o/CE+O6I | − | RN?? | NF− | 86.8 | |||
| 155 | WN6o+O9II/Ib | * | − | NF− | 116.6 | |||
| 156 | WN8h | − | − | |||||
| 157 | WN5o(+B1II) | − | − | |||||
Notes. WR designations by van der Hucht (2001); Spectral types from Harries et al. (1998); LE: line effect according to Harries et al. (1998) (+ line effect, * line effect due to binarity, − non-detection); RN: detections of ring nebulae, with classifications from Table 5; NF: detections of CS velocity displacements according to Nichols & Fesen (1994) (++ safe detection, + detection with possible super-shell, − non-detection); C iv: CS broadening velocities (FWHM in km s-1) from high-ionization features (average of C iv 1548, 1550 from Table 4).
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