Table 1.
Spectral classification of WR stars.
| Obj. ID | RA (J2000) | Dec (J2000) | Features/Reference | Classification |
|---|---|---|---|---|
| WR1 | 23:57:40.81 | −32:35:36.5 | (1) | WN2 |
| WR2 | 23:57:41.43 | −32:35:35.9 | (1) | WC4 |
| WR3 | 23:57:45.74 | −32:34:37.4 | Nebular lines + He II 4686 are weak, Hβ absorption | WN + O star |
| WR4 | 23:57:44.75 | −32:34:25.1 | N III 4640, He II 4886 | WN (late-type) |
| WR5 | 23:57:40.90 | −32:35:35.6 | He II 6560 (strong and broad) | WC4 |
| WR6 | 23:57:40.53 | −32:35:33.1 | N III 4640, He II 4686 | WN (late-type) |
| WR7 | 23:57:41.37 | −32:35:52.5 | N V 4603 + N III 4640 (in equal strength) | WN (mid-type) |
| WR8 | 23:57:43.27 | −32:35:49.6 | He II 4686 (narrow), N III 4640 | WN (late-type) |
| WR9 | 23:57:40.94 | −32:34:47.3 | Analogue to WR8, slightly broader He II | WN (late-type) |
References. (1) Bibby & Crowther (2010).
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