Todd M. Tripp, Limin Song
Using high-resolution ultraviolet spectra obtained with the HST/Space
Telescope Imaging Spectrograph (STIS) and the Far Ultraviolet Spectroscopic
Explorer, we study the metallicity, kinematics, and distance of the gaseous
"Outer Arm" (OA) and the high-velocity clouds (HVCs) in the outer Galaxy. We
detect the OA in a variety of absorption lines toward two QSOs, H1821+643 and
HS0624+6907. We search for OA absorption toward eight Galactic stars and detect
it in one case, which constrains the OA Galactocentric radius to 9View original: http://arxiv.org/abs/1101.1107
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