2002MNRAS.331..537L

We have found a bar of shocked molecular hydrogen (H₂) towards the OH(1720MHz) maser located at the projected intersection of supernova remnant (SNR) G359.1-0.5 and the non-thermal radio filament known as the Snake. The H₂ bar is well aligned with the SNR shell and almost perpendicular to the Snake. The OH(1720MHz) maser is located inside the sharp western edge of the H₂ emission, which is consistent with the scenario in which the SNR drives a shock into a molecular cloud at that location. The spectral line profiles of ¹² CO, HCO⁺ and CS towards the maser show broad-line absorption, which is absent in the ¹³ CO spectra and most probably originates from the pre-shock gas. A density gradient is present across the region and is consistent with the passage of the SNR shock, while the H₂ filament is located at the boundary between the pre-shock and post-shock regions.