We present a high-precision I-band light curve for the Wolf-Rayet binary WR 20a, obtained as a sub-project of the Optical Gravitational Lensing Experiment. Rauw et al. have recently presented spectroscopy for this system, strongly suggesting extremely large minimum masses of 70.7 +/- 4.0 Mo and 68.8 +/- 3.8 Mo for the component stars of the system, with the exact values depending strongly on the period of the system. We detect deep eclipses of about 0.4 mag in the light curve of WR 20a, confirming and refining the suspected period of P=3.686 days and deriving an inclination angle of i=74.5 +/- 2 deg. Using these photometric data and the radial velocity data of Rauw et al., we derive the masses for the two components of WR 20a to be 83.0 +/- 5.0 Mo and 82.0 +/- 5.0 Mo. Therefore, WR 20a is confirmed to consist of two extremely massive stars and to be the most massive binary known with an accurate mass determination.
@article{arxiv.astro-ph/0405338,
title = {WR 20a is an Eclipsing Binary: Accurate Determination of Parameters for an Extremely Massive Wolf-Rayet System},
author = {A. Z. Bonanos and K. Z. Stanek and A. Udalski and L. Wyrzykowski and K. Zebrun and M. Kubiak and M. K. Szymanski and O. Szewczyk and G. Pietrzynski and I. Soszynski},
journal= {arXiv preprint arXiv:astro-ph/0405338},
year = {2009}
}
Comments
13 pages, 2 figures, 3 tables, accepted for publication in ApJL