The RR Lyrae variable stars in the globular cluster IC 4499

Details The RR Lyrae variable stars in the globular cluster IC 4499 The RR Lyrae variable stars in the globular cluster IC 4499

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..217c&link_type=abstract

Astronomical Journal, vol. 84, Feb. 1979, p. 217-230.

Astronomy and Astrophysics

Astronomy

30

Cepheid Variables, Globular Clusters, Light Curve, Periodic Variations, Frequency Distribution, Histograms, Photographic Plates, Star Distribution, Stellar Magnitude

Scientific paper

Periods and light curves are presented for 75 RR Lyrae variables in the globular cluster IC 4499. Of these, 52 are of the ab type with a mean period of 0.578 + or - 0.009, and 23 are c type with a mean period of 0.351 + or - 0.004. The cluster belongs to Oosterhoff group I (the short-period group) and has the greatest frequency of RR Lyrae variables of the globular clusters in the Galaxy. The distribution of mean fundamentalized period and transition period and their correlation with Fe/H within globular clusters of similar horizontal-branch type to IC 4499 are discussed.

Affiliated with

Also associated with

No associations

Rating

The RR Lyrae variable stars in the globular cluster IC 4499 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 RR Lyrae variable stars in the globular cluster IC 4499, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The RR Lyrae variable stars in the globular cluster IC 4499 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828722