We present the first high-resolution spectra of the W UMa contact binary V524 Mon. The spectra of the two components are very similar, resembling a G5 and a K0. We find the radial velocities and rotational velocities consistent with corotation. We estimate the radii and the masses and derive a mass ratio M_2/M_1 = 2.1. We confirm that V524 Mon is a W-type contact system, likely enclosed in a common convective envelope, as found by Samec & Loflin (2003). We do not find evidence for the expected level of emission in the chromospheric CaII H and K lines, neither H_alpha, indicating that the magnetic activity is much weaker than expected or that other processes are hampering chromospheric emission.
@article{arxiv.astro-ph/0409200,
title = {First spectra of the W UMa system V524 Monocerotis},
author = {T. H. Dall and L. Schmidtobreick},
journal= {arXiv preprint arXiv:astro-ph/0409200},
year = {2009}
}