ZZ Ceti Stars: Fractal Analogues of Excited Helium Ions?

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dc.creatorOldershaw, R. L.
dc.date2006-02-20
dc.date.accessioned2026-07-07T07:00:48Z
dc.date.available2026-07-07T07:00:48Z
dc.descriptionMulti-periodic pulsation phenomena of ZZ Ceti variable stars are analyzed within the context of a fractal cosmological paradigm that emphasizes discrete self-similarity in nature. A quantitative test comparing relevant stellar and atomic periods provides preliminary support for the analysis. This paper completes a 3-part series that explores the possibility of discrete cosmological self-similarity in variable stars; the first and second papers discussed RR Lyrae and delta Scuti stars, respectively.
dc.description17 pages, 4 figures, 7 tables, comments welcome
dc.identifierhttps://arxiv.org/abs/astro-ph/0602451
dc.identifierhttp://arxiv.org/abs/astro-ph/0602451
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108090
dc.subjectAstrophysics
dc.titleZZ Ceti Stars: Fractal Analogues of Excited Helium Ions?
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