High-Velocity Molecular Gas in the Galactic Center Radio Lobe
Abstract
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 +100 , and the western spur approaching at -150 , suggesting a high-velocity rotation of the GCL. We study the kinematics of the GCL based on these molecular line data.
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