The Blazhko behavior of RV UMa

Details The Blazhko behavior of RV UMa The Blazhko behavior of RV UMa

2007-08-14

arxiv.org/abs/0708.1863v1

Astronomy and Astrophysics

Astrophysics

4 pages, 5 figures, accepted for publication in AN

Scientific paper

10.1002/asna.200710815

RV UMa is one of the most extensively studied RR Lyrae stars showing Blazhko modulation. Its photometric observations cover more than 90 years. The published photoelectric observations of RV UMa obtained at the Konkoly Observatory (Kanyo, 1976) were re-considered and completed with previously unpublished data. During the time interval of the observations the periods of both the pulsation and the modulation varied within the ranges of 0.000007 and 0.9 days, respectively. We have found a definite but not strict inverse relation between the pulsation and modulation periods of RV UMa.

Affiliated with

Also associated with

No associations

Rating

The Blazhko behavior of RV UMa 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 behavior of RV UMa, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Blazhko behavior of RV UMa will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-389460