Publication | Open Access
Constraining the Evolution of ZZ Ceti
40
Citations
40
References
2003
Year
We report our analysis of the stability of pulsation periods in the DAV star (pulsating hydrogen atmosphere white dwarf) ZZ Ceti, also called R548. On the basis of observations that span 31 years, we conclude that the period 213. 13 s observed in ZZ Ceti
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