The Blazhko Effect in RR Lyrae stars: Strong observational support for the oblique pulsator model in three stars

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dc.creatorThe MACHO Collaboration
dc.creatorAlcock, C.
dc.creatorAlves, D. R.
dc.creatorBecker, A.
dc.creatorBennett, D. P.
dc.creatorCook, K. H.
dc.creatorFreeman, K. C.
dc.creatorGriest, K.
dc.creatorKurtz, D. W.
dc.creatorLehner, M. J.
dc.creatorMarshall, S. L.
dc.creatorMinniti, D.
dc.creatorPeterson, B. A.
dc.creatorPratt, M. R.
dc.creatorQuinn, P. J.
dc.creatorRodgers, A. W.
dc.creatorSutherland, W.
dc.creatorTomaney, A.
dc.creatorVandehei, T.
dc.creatorWelch, D. L.
dc.date1998-08-19
dc.date.accessioned2026-07-07T02:27:39Z
dc.date.available2026-07-07T02:27:39Z
dc.descriptionUsing the novel data set of the MACHO project, we show that three ``Blazhko Effect'' RR Lyrae stars show nearly-pure amplitude modulation of a single pulsation mode. This is strong observational evidence that the ``Oblique Pulsator Model'' is the correct solution to this 90-year-old problem.
dc.description31 pages, 9 Encapsulated PostScript figures. Submitted to the Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/9808190
dc.identifierhttp://arxiv.org/abs/astro-ph/9808190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12786
dc.subjectAstrophysics
dc.titleThe Blazhko Effect in RR Lyrae stars: Strong observational support for the oblique pulsator model in three stars
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