The Blazhko Effect of RR Lyrae in 1996

Details The Blazhko Effect of RR Lyrae in 1996 The Blazhko Effect of RR Lyrae in 1996

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasp..115...43s&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 115, Issue 803, pp. 43-48.

Other

28

Stars: Variables: Other

Scientific paper

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 fB is the Blazhko frequency.

Affiliated with

Also associated with

No associations

Rating

The Blazhko Effect of RR Lyrae in 1996 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Blazhko Effect of RR Lyrae in 1996, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Blazhko Effect of RR Lyrae in 1996 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1321211