**Table 2:** Model parameters, cf. Sect. 3.2. The model names are given in Col. 1. Starting from the left the remaining columns specify: the stellar luminosity L_*; the effective temperature $\ensuremath{T_{\mathrm{eff}}}$ ; the pulsation period P; the pulsation amplitude $\ensuremath{\Delta\,u_{\mathrm{p}}}$ ; and the carbon/oxygen ratio $\ensuremath{\varepsilon_{\mathrm{C}}/\varepsilon_{\mathrm{O}}}$ . The stellar mass M_* is set to $1.0\,M_{\hbox {$\odot $ }}$ in all models.
model	L_*	$\ensuremath{T_{\mathrm{eff}}}$	P	$\ensuremath{\Delta\,u_{\mathrm{p}}}$	$\ensuremath{\varepsilon_{\mathrm{C}}/\varepsilon_{\mathrm{O}}}$
	$[L_{\hbox{$\odot$ }}]$	$[\mbox{K}]$	$[\mbox{d}]$	$[\!\ensuremath{\,\mbox{km}\,\mbox{s}^{-1}} ]$
P13C16U6	$1.3\times10^4$	2700	650	6	1.6
P13C14U6	$1.3\times10^4$	2700	650	6	1.4
P10C18U4	$1.0\times10^4$	2790	525	4	1.8

Source LaTeX | All tables | In the text