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This study investigates the blue straggler star (BSS) population in the Galactic globular cluster M75 (NGC 6864) using high-resolution and wide-field observations. A total of 62 bright BSSs were identified, showing a significant concentration in the cluster core, with no observed increase in frequency in the outskirts, contrasting with other clusters. The findings suggest that most heavy stars have sunk to the core, indicating a strong mass segregation effect within M75.

Author
elpericles
Language
EN

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