ORIGIN(S) OF THE HIGHLY IONIZED HIGH-VELOCITY CLOUDS BASED ON THEIR DISTANCES

Previous Hubble Space Telescope and FUSE observations have revealed highly ionized high-velocity clouds (HVCs) or more generally low Hi column HVCs along extragalactic sight lines over 70%-90% of the sky. The distances of these HVCs have remained largely unknown hindering from distinguishing a Galactic origin (e. g., outflow, inflow) from a Local Group origin (e. g., warm-hot intergalactic medium). We present the first detection of highly ionized HVCs in the Cosmic Origins Spectrograph spectrum of the early-type star HS 1914+7134 (l = 103 degrees, b = +24 degrees) located in the outer region of the Galaxy at d similar or equal to 14.9 kpc. Two HVCs are detected in absorption at upsilon(LSR) = -118 and -180 km s(-1) in several species, including C IV, Si IV, Si III, Al II, C II, Si II, O I, but H I 21 cm emission is only seen at -118 km s(-1). Within 17 degrees of HS 1914+7134, we found HVC absorption of low and high ions at similar velocities toward five extragalactic sight lines, suggesting that these HVCs are related. The component at -118 km s(-1) is likely associated with the outer arm of the Milky Way. The highly ionized HVC at -180 km s(-1) is possibly an HVC plunging at high speed onto the thick disk of the Milky Way. This is the second detection of highly ionized HVCs toward Galactic stars, supporting a Galactic origin for at least some of these low Hi column density HVCs.