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Table 11
High-resolution average Praesepe (NGC 2632) abundances.
Here | P08a | A07b | Bu98c | ||
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R = λ/δλ | 30 000 | 100 000 | 55 000 | 90 000 | |
S/N | 50–100 | ≃80 | ≃100 | ~200 | |
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[Fe/H] | +0.16 ± 0.05 | +0.27 ± 0.10 | +0.11 ± 0.03 | +0.40 ± 0.14 | |
[Al/Fe] | +0.00 ± 0.03 | –0.05 ± 0.12 | – | –0.19 ± 0.17 | |
[Ba/Fe] | +0.33 ± 0.05 | +0.22 ± 0.06 | – | – | |
[Ca/Fe] | –0.08 ± 0.02 | +0.00 ± 0.11 | – | +0.04 ± 0.16 | |
[Co/Fe] | +0.04 ± 0.02 | – | – | – | |
[Cr/Fe] | +0.05 ± 0.01 | –0.01 ± 0.08 | – | – | |
[La/Fe] | –0.05 ± 0.02 | – | – | – | |
[Mg/Fe] | +0.27 ± 0.05 | – | – | – | |
[Na/Fe] | +0.25 ± 0.06 | –0.04 ± 0.12 | – | – | |
[Ni/Fe] | +0.02 ± 0.02 | –0.02 ± 0.12 | – | +0.21 ± 0.17 | |
[O/Fe] | –0.11 ± 0.03 | –0.40 ± 0.20 | – | – | |
[Sc/Fe] | –0.04 ± 0.05 | – | – | – | |
[Si/Fe] | +0.06 ± 0.02 | –0.01 ± 0.12 | – | – | |
[Ti/Fe] | –0.07 ± 0.03 | –0.04 ± 0.12 | – | – | |
[V/Fe] | +0.06 ± 0.03 | – | – | – | |
[Y/Fe] | –0.11 ± 0.01 | – | – | – |
Notes.
(a)
Pace et al. (2008), from 6 G and 1 F main sequence stars.
(b)
An et al. (2007), from 4 G dwarfs stars.
(c)
Burkhart & Coupry (1998), from 10 Am stars.
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