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Constraining the Evolution of ZZ Ceti

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Mukadam, Anjum; Kepler, S O; Winget, D E; Nather, R E; Kilic, M; Mullally, F; von Hippel, Ted; Kleinman, S; Nitta, A; Guzik, J A; Bradley, P A; Matthews, J M; Sekiguchi, K; Sullivan, D J; Sullivan, T; Shobbrook, R; Birch, P V; Jiang, X; Xu, D W; Joshi, S; Ashoka, B N; Ibbetson, P; Leibowitz, E; Ofek, Eran O; Meistas, E; Janulis, R; Alisauskas, D; Kalytis, R; Handler, G; Kilkenny, D; O'Donoghue, D; Kurtz, D W; Muller, M; Moskalik, P; Ogloza, W; Zola, S; Krzesinski, J; Johannessen, F; Gonzalez-Perez, J; Solheim, Jesper; Silvotti, R; Bernabei, S; Vauclair, G; Dolez, N; Fu, J; Chevreton, M; Mantiega, M; Suarez, O; Ulla, A; Cunha, M S; Metcalfe, T S; Kanaan, A; Fraga, L; Costa, A F M; Giovannini, O; Fontaine, G; Bergeron, P; O'Brien, M S; Sanwal, D; Wood, M A; Ahrens, T J; Silvestri, Nicole; Klumpe, E W; Kawaler, S D; Riddle, R L; Reed, M D; Watson, T K

Description

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

CollectionsANU Research Publications
Date published: 2003
Type: Journal article
URI: http://hdl.handle.net/1885/86678
Source: Astrophysical Journal, The
DOI: 10.1086/377044

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