Table 2
Evolved stars in the Carina region.
| Name | Type | Cluster | Initial mass | 26Al |
| M⊙ | (10-4 M⊙) | |||
|
|
||||
| HD 92809 | WC6 | Bochum 10 | ~30 | 0.3–1.5 |
| HD 92964 | B2 Ia | Bochum 10 | ~30 | 0.0–0.3 |
| HD 92852 | K1/3 III | Bochum 10 | ~30 | 0.0–0.3 |
| Evans 3293-001 | B0 Iab | NGC 3293 | ~20 | 0.0–0.1 |
| Evans 3293-002 | B0.7 Ib | NGC 3293 | ~20 | 0.0–0.1 |
| Feinstein CPD 3502 | M1.5 Iab-Ib | NGC 3293 | ~20 | 0.0–0.1 |
| HD 93129Aa | O2 If | Trumpler 14 | 80-120 | 0.0–4.0 |
| η Car | LBV | Trumpler 16 | 80–120 | 0.0–4.0 |
| HD 93162 | WN6ha | Trumpler 16 | 80–120 | 2.0–8.0 |
| HD 93131 | WN6ha | Trumpler 16 | 80–120 | 2.0–8.0 |
| HD 92740A | WN7ha | Trumpler 16 | 80-120 | 2.0–8.0 |
| Hucht WR27 | WC6 | Field (2.5) | – | – |
| HD 94546 | WN4 | Field (4.05) | – | – |
| Hucht WR31a | WN11h | Field (8.0) | – | – |
| HD 90657 | WN5 | Field (3.88) | – | – |
| HD 95435 | WC5 | Field (6.11) | – | – |
| Hucht WR21a | WN6 | Field (?) | – | – |
Notes. Stars without HD designations are labelled by the name of the first author of the publication in which they appear (see Sect. 3), followed by the name given in that publication. The initial masses are estimated by the maximum mass of stars still present in a population with the age of the host cluster. The ejected amount of 26Al is found from the stellar tracks at the given mass. The range is over all WR-phases for WR-stars, and until the onset of the WR-winds for non-WR stars.
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