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Constraining the Evolution of ZZ Ceti

40

Citations

40

References

2003

Year

Abstract

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

References

YearCitations

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