We study the radial-velocity and light curves of the two eclipsing binaries EE Aqr and Z Vul. Using the latest version of the Wilson & Van Hamme (2003) model, absolute parameters for the systems are determined. We find that EE Aqr and Z Vul are near-contact and semi-detached systems, respectively. The primary component of EE Aqr fills about 96% of its 'Roche lobe', while its secondary one appears close to completely filling this limiting volume. In a similar way, we find fill-out proportions of about 72 and 100% of these volumes for the primary and secondary components of Z Vul respectively. We compare our results with those of previous authors.
@article{arxiv.0805.0489,
title = {Reanalysis of two eclipsing binaries: EE Aqr and Z Vul},
author = {Sayyed Mohammad Reza Ghoreyshi and Jamshid Ghanbari and Fatemeh Salehi},
journal= {arXiv preprint arXiv:0805.0489},
year = {2009}
}