Monitoring the Polarisations of the Hydroxyl Masers in the Periodic Methanol Maser Source G9.62 + 0.20E

This study investigates the environment of the high mass star forming region G9.62 + 0.20E by employing the monitoring of galactic hydroxyl and methanol masers known to be associated with this natal phase.A monitoring campaign was instituted to study the left and right circular polarization components of the 1.6 GHz mainline hydroxyl masers and the 6.7 GHz methanol masers.This campaign revealed continual variability of the flux density of the 6.7 GHz methanol masers and the left and right circular polarization components of the 1.6 GHz OH mainline masers.