OVI Velocity Distribution in the LSR

The Sample: • 103 FUSE Obs. Of AGN • 54 with S/N  5 per Res. El., at 1032 Å • 45 show at least 1 OVI abs. at z~0, at our detection threshold (7 of the remaining 9 have poor S/N spectra) • 38/45 LV-OVI • 32/45 HV-OVI • 21 both • High Covering Factor (could be 90 % down to 20 mÅ, Sembach et al., 2002)

Low Velocity (LV)

High Velocity (HV)

High Velocity (HV)

MSSL, 24-25 October 2002