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<q<0.35), luminosity ratio (L1/L2 about 4.0) and the ratio of the radii of the components (r1/r2 about 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.
@article{arxiv.0910.5609,
title = {An Unusual Eclipsing Blue Straggler V8-NGC 6752},
author = {J. Kaluzny and M. Rozyczka and I. B. Thompson and K. Zloczewski},
journal= {arXiv preprint arXiv:0910.5609},
year = {2009}
}
Comments
13 pages, 5 figures, submitted to Acta Astronomica