Table 2.
SNRs, PNe, and WRs identified in the MUSE FoV and reference to previous detections.
| Obj. ID | RA (J2000) | Dec (J2000) | Ref. | Ref. ID |
|---|---|---|---|---|
| SNR1 | 23:57:43.82 | −32:35:27.8 | (1) | N7793-S6 |
| SNR2 | 23:57:45.80 | −32:35:01.9 | (1) | N7793-S10 |
| SNR3 | 23:57:44.00 | −32:35:32.1 | ||
| PN1 | 23:57:42.71 | −32:35:39.2 | ||
| PN2 | 23:57:44.01 | −32:34:41.2 | ||
| WR1 | 23:57:40.81 | −32:35:36.5 | (2) | 10 (WN2-4b) |
| WR2 | 23:57:41.43 | −32:35:35.9 | (2) | 14 (WC4) |
| WR3 | 23:57:45.74 | −32:34:37.4 | ||
| WR4 | 23:57:44.75 | −32:34:25.1 | ||
| WR5 | 23:57:40.90 | −32:35:35.6 | ||
| WR6 | 23:57:40.53 | −32:35:33.1 | ||
| WR7 | 23:57:41.37 | −32:35:52.5 | ||
| WR8 | 23:57:43.27 | −32:35:49.6 | ||
| WR9 | 23:57:40.94 | −32:34:47.3 |
Notes. Spectra of all candidates can be found in the appendix.
References. (1) Pannuti et al. (2002); (2) Bibby & Crowther (2010).
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