Asteroseismology of ZZ Ceti stars with full evolutionary white dwarf models - II. The impact of AGB thermal pulses on the asteroseismic inferences of ZZ Ceti stars

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Table 1

Spectroscopic determinations of T_eff and M_wd∕M_⊙ corresponding to the ZZ Ceti stars selected in this work.

Star	T_eff	M_wd∕M_⊙	Reference
KUV 11370+4222	11 890	0.639	Bergeron et al. (2004)
HE 0031−5525	11 480	0.44	Castanheira et al. (2006)
WD J1002+5818	11 710	0.57	Mullally et al. (2005)
WD J0214−0823	11 570	0.57	Mukadam et al. (2004)
BPM 31594	11 450	0.666	Bergeron et al. (2004)
G191−16	11 420	0.632	Bergeron et al. (2004)
MCT 0145−2211	11 500	0.684	Bergeron et al. (2004)
WD J150−0001	11 200	0.61	Mukadam et al. (2004)
HE 1429−037	11 434	0.514	Silvotti et al. (2005)
EC 23487−2424	11 520	0.661	Bergeron et al. (2004)
G232−38	11 350	0.610	Gianninas et al. (2006)

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