Low mass ratio contact binary systems are more likely to have unstable orbits and
potentially merge. In addition, such systems exhibit characteristics such as starspots and high
energy emissions (UV) suggestive of chromospheric and magnetic activity. Light curve modelling
of ten contact binary systems is reported. All were found to be of extreme low mass
ratio ranging from 0.122 to 0.24 and three were found to be potentially unstable and possible
merger candidates. Filling of the infrared Calcium absorption lines is a marker of increased
chromospheric activity. We use the available LAMOST spectra along with matched standard
spectra (broadened for rotation) to measure the excess filling of the central core depression
flux of the two main infrared Calcium absorption lines λ8542 and λ8662. We find that all
reported contact binaries have excess filling of the core flux in the infrared Calcium lines.
Three of the systems reported were also observed by the GALEX mission and we find that all
three have features of excess ultraviolet emissions further adding evidence for increased chromospheric
activity in low mass ratio contact binaries. Analysis of both orbital stability and
absorption line filling is dependent on the determination of geometric and absolute parameters
from light curve modelling. Not an insignificant number of contact binary light curves exhibit
the O’Connell effect, usually attributed to starspots. We discuss the inclusion of starspots in
light curve solutions and how they influence the geometric and absolute parameters.