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Home All issues Volume 508 / No 3 (December IV 2009) A&A, 508 3 (2009) 1359-1374 Full HTML
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Table 3:

Percentage of CEMP, NEMP and FEMP (sub-)giants relative to total EMP giants in our model binary populations of Table 1.

Model Set 		CEMP/EMP $\%$ NEMP/EMP $\%$ FEMP/EMP $\%$ CEMP-s/CEMP $\%$
A $2.30 \pm 0.04$ $0.267 \pm 0.007$ 2.03 28.3
Ap7 $2.99 \pm 0.04$ $0.267 \pm 0.005$ 2.03 21.8
Ap5 $3.46 \pm 0.04$ $0.267 \pm 0.005$ 2.03 18.8
A1 $2.30 \pm 0.04$ $0.267 \pm 0.007$ 2.03 86.3
A2 $2.30 \pm 0.04$ $0.267 \pm 0.007$ 2.03 94.1
B $3.05 \pm 0.04$ $0.323 \pm 0.006$ 2.74 47.2
C $2.94 \pm 0.04$ $0.311 \pm 0.007$ 2.36 29.1
D $4.21 \pm 0.04$ $0.409 \pm 0.004$ 3.74 63.1
E $2.90 \pm 0.04$ $0.267 \pm 0.007$ 2.43 43.5
F $6.47 \pm 0.03$ $0.267 \pm 0.006$ 5.16 22.3
G $9.43 \pm 0.04$ $0.266 \pm 0.006$ 7.81 94.1
H $15.52 \pm 0.07$ $0.426 \pm 0.004$ 13.5 97.2

(See Sect. 2.6 for selection criteria and Table D.2 for the full set of results.) The errors convey Poisson statistics only. The final column gives the number ratio of CEMP-s to CEMP stars.


Source LaTeX | All tables | In the text

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