Hubble Space Telescope reveals multiple Sub-Giant Branch in eight Globular Clusters

TL;DR

This study uses high-precision Hubble Space Telescope photometry to identify multiple sub-giant branches in eight globular clusters, revealing complex stellar populations and potential age or chemical composition differences.

Contribution

It provides new evidence of multiple sub-giant branches in several globular clusters, expanding understanding of their complex stellar populations.

Findings

Multiple SGBs detected in eight globular clusters.

Variation in the fraction of faint SGB stars across clusters.

Consistent magnitude difference suggests age or chemical composition differences.

Abstract

In the last few years many globular clusters (GCs) have revealed complex color-magnitude diagrams, with the presence of multiple main sequences (MSs), broaden or multiple sub-giant branches (SGBs) and MS turn offs, and broad or split red giant branches (RGBs). After a careful correction for differential reddening, high accuracy photometry with the Hubble Space Telescope presented in this paper reveals a broadened or even split SGB in five additional Milky Way GCs: NGC 362, NGC 5286, NGC 6656, NGC 6715, and NGC 7089. In addition, we confirm (with new and archival HST data) the presence of a split SGB in 47Tuc, NGC 1851, and NGC 6388. The fraction of faint SGB stars with respect to the entire SGB population varies from one cluster to another and ranges from $\sim$0.03 for NGC 362 to ~0.50 for NGC 6715. The average magnitude difference between the bright SGB and the faint SGB is almost the same at different wavelengths. This peculiarity is consistent with the presence of two groups of stars with either an age difference of about 1-2 Gyrs, or a significant difference in their overall C+N+O content.