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High-Velocity Molecular Gas in the Galactic Center Radio Lobe

We point out a possible association of high-velocity molecular gas with the Galactic center radio lobe (GCL). A molecular spur in the eastern GCL ridge is receding at VLSR ~ +100 km s-1, and the western spur approaching at VLSR ~ -150 km s-1, suggesting a high-velocity rotation of the GCL. We study the kinematics of the GCL based on these molecular line data.