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Table 7
Abundance analyses of Collinder 261 stars – approximate number of Fe I and Fe II lines used per star, and corresponding wavelength ranges.
| Fe I | Fe II | |||
| Reference | n | λ [nm] | n | λ [nm] |
|
|
||||
| Friel et al. (2003) | 40 | 538–785 | 8 | 541–652 |
| Carretta et al. (2005) | 100 | 550–700 | 10 | 550–700 |
| De Silva et al. (2007) | 60 | 422–620 | 12 | 449–615 |
| Sestito et al. (2008) | 100 | 550–681 | 13 | 553–652 |
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