Uncertainties on the theoretical predictions for classical Cepheid pulsational quantities

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Table 1:

Computed sets of evolutionary tracks and pulsation models.
Case	Y	Z	Mixture
I (std)	0.26	0.005	AGS05
II ( $Z_{\rm low}$ )	0.26	0.0035	AGS05
III ( $Z_{\rm high}$ )	0.26	0.008	AGS05
IV ( $Y_{\rm high}$ )	0.28	0.005	AGS05
V ( $Y_{\rm high}$ , $Z_{\rm high}$ )	0.28	0.008	AGS05
VI ( $Z_{\rm high}$ , GS98)	0.26	0.008	GS98
VII (¹²C( $\alpha$ , $\gamma$ )¹⁶O) $_{\rm high}$	0.26	0.005	AGS05
VIII (¹²C( $\alpha$ , $\gamma$ )¹⁶O) $_{\rm low}$	0.26	0.005	AGS05
IX (¹⁴N(p, $\gamma$ )¹⁵O) $_{\rm high}$	0.26	0.005	AGS05
X (¹⁴N(p, $\gamma$ )¹⁵O) $_{\rm low}$	0.26	0.005	AGS05
XI ( $l_{\rm ov}=0.1 H_{\rm p}$ )	0.26	0.005	AGS05
XII ( $l_{\rm ov}=0.25 H_{\rm p}$ )	0.28	0.005	AGS05
XIII ( $l_{\rm ov}=0.25 H_{\rm p}$ )	0.26	0.005	AGS05

GS98 = Grevesse & Sauval (1998), AGS05 = Asplund et al. (2005).

Source LaTeX | All tables | In the text

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