Population synthesis of binary carbon-enhanced metal-poor stars

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Table 1:

Physical parameters corresponding to the most important of our binary population models. (A full list of all our model sets can be found in Table D.1.)
Model set	Physical parameters
	(differences from model set A)
A	-
Ap5, Ap7	$\left[{\rm C}/{\rm Fe}\right]_{{\rm min}}=0.5$ and 0.7respectively
A1, A2	$\xi_{13}=0.1$ and 0.01 respectively
B	Bondi-Hoyle efficiency $\alpha_{{\rm BH}}=5$
C	common envelope accretion $0.05~M_{\odot}$
D	no thermohaline mixing
E	$\Delta M_{{\rm c,min}}=-0.07~M_{\odot}$ , $\lambda_{{\rm min}}=0.8$
F	$M_{{\rm env},{\rm min}}=0~M_{\odot}$
G	$\Delta M_{{\rm c,min}}=-0.1~M_{\odot}$ , $\lambda_{{\rm min}}=0.8$ ,
	$M_{{\rm env},{\rm min}}=0~M_{\odot}$ , $\xi_{{\rm 13}}=0.1$
H	as model G, with:
	common envelope accretion $0.05~M_{\odot}$
	no thermohaline mixing

Source LaTeX | All tables | In the text

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