Revisiting the Evidence for Double Sequences of Blue Straggler Stars in Globular Clusters

Abstract Blue straggler stars (BSSs) are believed to form through mass transfer in binary systems or stellar collisions. The reported presence of double BSS sequences in some globular clusters (GCs) has been interpreted as evidence that these two formation channels produce distinct sequences in color–magnitude diagrams. We reassess this claim using Hubble Space Telescope (HST) UV Globular Cluster Survey photometry of 56 Galactic GCs. We used the Hartigan dip test to test bimodality, and Akaike model comparison to test whether BSS distance distributions are better described by a mixture of two unskewed Gaussians or a skewed unimodal Gaussian model. We find no strong statistical evidence for bimodality: no cluster yields a dip test p -value below 0.15, and the Akaike model comparison favors the skewed unimodal model in 94 out of 112 cases. We reexamine NGC 7099 (M30), the prototypical case of a double BSS sequence, using three reductions of HST data. We find bimodality is detected at p = 4 × 10 −3 , versus the originally reported p ∼ 10 −5 , in the original photometry. The observed uncertainties derived from the subgiant branch widths are comparable to the suggested separation between the proposed BSS sequences, making the detection of statistically significant bimodality challenging. Our results suggest that the dip between two BSS sequences in the M30 photometry is a coincidence, and that later bifurcation claims can be explained as skew in the BSS color distribution, rather than two separate distributions.