An Unusual Eclipsing Blue Straggler V8-NGC 6752

We report the analysis of a binary blue straggler in NGC 6752 with a short orbital period of 0.315 d and a W UMA-type light Curve. We use photometric data spanning 13 years to place limits on the mass ratio (0.15 less than or similar to q less than or similar to 0.35), luminosity ratio (L-1/L-2 approximate to 4.0) and the ratio of the radii of the components (r(1)/r(2) approximate to 2.0). The effective temperatures of the components are nearly identical, and the system is detached or semi-detached (in the latter case the component filling its Roche lobe is the secondary). Such a configuration is unusual given the shortness of the orbital period, and it must have resulted from Substantial mass exchange. We suggest that some secondaries of W UMa-type stars, normally regarded as main sequence objects which fill their Roche lobes to different degrees, in fact may be shell-burning cores of originally more massive components.