Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..43...47t&link_type=abstract
Astrophysics and Space Science, Volume 43, Issue 1, pp.47-55
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
Integrated colors of M3, M5, M13, and M92 are calculated from the luminosity function, the color-magnitude diagram, and the two-color diagram to compare them with observed ones. The results show good agreements for M3, M13, and M92 and the discrepancy for M5. Possible causes for this discrepancy are discussed. To study the way in which integrated colors are affected by changes in the distribution of stars in the color-magnitude diagram, we calculate the integrated colors by taking into account changes in the distribution of horizontal branch stars and in the ratio of the number of horizontal branch stars to that of red giant branch stars. The result shows that (B-V) color varies within the range of about 0.1 mag with changes in the distribution of horizontal branch stars, implying that the cluster with a well-developed blue horizontal branch has bluer intrinsic integrated (B-V) color than that with yellow one. This tendency is compared with observation.
Kaneko Noboru
Nishimura Masaki
Toyama Kiyotaka
No associations
LandOfFree
Integrated Colors of Globular Clusters 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 Integrated Colors of Globular Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Integrated Colors of Globular Clusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1872363