Publication
Title
The Blazhko effect of RR Lyrae in 1996
Author
Abstract
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.
Language
English
Source (journal)
Publications of the Astronomical Society of the Pacific. - San Francisco, Calif., 1889, currens
Publication
San Francisco, Calif. : 2003
ISSN
0004-6280 [print]
1538-3873 [online]
DOI
10.1086/345458
Volume/pages
115 :803 (2003) , p. 43-48
ISI
000180000300005
Full text (Publisher's DOI)
Full text (publisher's version - intranet only)
UAntwerpen
Publication type
Subject
External links
Web of Science
Record
Identifier
Creation 26.04.2018
Last edited 18.08.2024
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