Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars

Details Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars

2010-10-06

arxiv.org/abs/1010.1119v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

19 pages, 27 figures, MNRAS accepted

Scientific paper

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in two additional cases. The mean pulsation period of Blazhko stars is 0.04 d shorter than the mean period of the entire RRab sample in M5. Among the RRab stars with period shorter than 0.55 d the incidence rate of the modulation is as high as 60 per cent. The mean $B-V$ colours of Blazhko stars overlap with the colours of first overtone RRc (RR1) pulsators. The mean $V$ magnitudes of Blazhko stars are on the average 0.05-mag fainter than those of the RRab stars with stable light curves. Blazhko stars tend to be situated close to the zero-age horizontal branch at the blue edge of the fundamental-mode instability strip in M5. We speculate that this specific location hints that the Blazhko effect may have an evolutionary connection with the mode switch from the fundamental to the overtone-mode pulsation.

Affiliated with

Also associated with

No associations

Rating

Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars 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 Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-427470