On the Nature of Bright Blue Stragglers in the Centre of m3 and NGC6397 - Analysis of UBV Observations

Astronomy and Astrophysics – Astrophysics

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Globular Clusters: Individual: M 3, Ngc 6397, Stars: Population Ii-Stars: Evolution, Techniques: Photometric

Scientific paper

We present UBV CCD observations of the central region of the globular cluster M 3 obtained with the 2 m Bernard Lyot telescope of Pic-du-Midi observatory under V subarcsecond seeing conditions. The V vs. B-V diagram reveals at least 8 bright blue stragglers (BSs) to exist in the 4O"x12O" investigated field. The UBV M 3 data are analysed together with those obtained for NGC 6397 (Lauzeral et al. 1992) in order to check the origin of the bright central BSs. Using a suggestion from Bailyn (1992), we adopt sufficient conditions for a BS to have a collisional origin. Effects of stellar evolution are also taken into account. At least two of the central NGC 6397 BSs verify these sufficient conditions, and all may lie on a post turnover sequence. This strengthens the hypothesis that those stars result from collisions in the very dense core of NGC 6397. As to the more distant cluster M 3, two of the central BSs have photometric properties of the collisional ones, but errors on the magnitudes prevent any firm conclusion to be derived.

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