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Table 2.
Clusters in ESO 338 with WR features.
| IDa | Age | Mass | Cov. | Blue | Red |
|---|---|---|---|---|---|
| (Myr) | (105 M⊙) | fraction | bump | bump | |
| 23 | 4 | 38 | 0.0 | Y | Y |
| 18 | 3–6 | 2.4–4.5 | 0.0–0.5 | Y | Y |
| 50/51b | 3–4 | 0.8–1.3 | 0.5–1.0 | Y | Y |
| 53 | 3–4 | 3.6–4.0 | 0.5–1.0 | Y | N |
Notes.
(a)
IDs taken from Östlin et al. (1998).
(b)
This source was resolved by Östlin et al. (1998) in two clusters, while with the new fitting, it was selected as 1 extended source.
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