High-Velocity Molecular Gas in the Galactic Center Radio Lobe

Details High-Velocity Molecular Gas in the Galactic Center Radio Lobe High-Velocity Molecular Gas in the Galactic Center Radio Lobe

1995-12-28

arxiv.org/abs/astro-ph/9512162v1

Astronomy and Astrophysics

Astrophysics

To appear in ApJ. Letters, Plain TeX, Figures on request

Scientific paper

10.1086/309946

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 $\Vlsr \sim +100$ \kms, and the western spur approaching at $\Vlsr
\sim -150$ \kms, 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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