Table 2: Objects which do not show pulsations.
Name RA2000 Dec2000 B $T_{\rm eff}$ $\log g$ UT date D L
        (K) (cgs) at start (h) (mma)
HS 1253+1033 12 56 28.5 +10 17 09 14.4 12 600 8.5 16/06/04 1.6 5.3
HS 1443+2934 14 45 28.5 +29 21 31 14.5 12 400 8.1 22/06/04 2.0 1.5
            23/06/04 1.5 1.2
HS 1610+1639 16 13 02.4 +16 31 56 15.8 14 500 8.4 17/06/04 3.4 2.0
HS 1641+7132 16 41 00.0 +71 26 59 16.7 15 300$^{\ast}$ 7.9$^{\ast}$ 23/06/04 1.4 4.6

$^{\ast}$ An alternative solution for this star gives $\mbox{$T_{\rm eff}$ }=11~600$ K and $\mbox{$\log g$ }=8.0$ (see Sect. 2.2 for more details).


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Selection of the ZZ Ceti candidates
3 Time-series photometry
4 The ZZ Ceti instability strip updated
References
List of tables
List of figures