Table 3
CEMP star frequencies.
| Fe/H] ≤ | % CEMP stars | ||
| Scl dSph | Dwarfs | MW Halo | |
|
|
|||
| –2.0 | 2 (3) | 8 | 43 |
| –2.5 | 0 (4) | 22 | 44 |
| –3.0 | 0 (8) | 40 | 50 |
| –3.5 | 0 (17) | 50 | 62 |
Notes. Fraction of CEMP stars (percent; according the Aoki et al. 2007 criterion) per metallicity bins for Scl dSph; dwarf galaxies in the Local Group; and the Galactic halo. The same literature data are plotted in Fig. 12. The values in parenthesis refer to the fraction of CEMP stars in Scl when taking the [C/Fe] upper limit from Frebel et al. (2010) into account for star S102549, with [Fe/H] = –3.8 dex and [C/Fe] = +0.16 dex.
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