Title
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The Blazhko effect of RR Lyrae in 1996
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Author
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Abstract
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Photoelectric B and V photometry of RR Lyrae was obtained over a 77 day interval in 1996. In addition to the 0.5668 day primary period, RR Lyr displayed a prominent 40 day Blazhko cycle during this time span. The observed light curve can be well but not perfectly described by frequency triplets of the form kf(0) + jf(B), where, k = 0, 1, 2, ..., j = 1, 0, 1, f(0) is the primary pulsation frequency, and f(B) is the Blazhko frequency. |
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Language
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English
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Source (journal)
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Publications of the Astronomical Society of the Pacific. - San Francisco, Calif., 1889, currens
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Publication
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San Francisco, Calif.
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2003
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ISSN
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0004-6280
[print]
1538-3873
[online]
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DOI
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10.1086/345458
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Volume/pages
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115
:803
(2003)
, p. 43-48
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ISI
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000180000300005
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Full text (Publisher's DOI)
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Full text (publisher's version - intranet only)
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