Constraining the Evolution of ZZ Ceti
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Altmetric Citations
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
Collections | ANU Research Publications |
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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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