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2003PASP..115...43S - Publ. Astron. Soc. Pac., 115, 43-48 (2003/January-0)

The Blazhko effect of RR Lyrae in 1996.

SMITH H.A., CHURCH J.A., FOURNIER J., LISLE J., GAY P., KOLENBERG K., CARNEY B.W., DICK I., PETERSON R.C. and HAKES B.

Abstract (from CDS):

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 kf0+jfB, where k=0, 1, 2,..., j=-1, 0, 1, f0 is the primary pulsation frequency, and fBis the Blazhko frequency.

Abstract Copyright: ∼

Journal keyword(s): Stars: Variables: Other

Simbad objects: 8

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