activity
19952024
most citedOverview of the Far Ultraviolet Spectroscopic Explorer Mission

665 citations · 8.9k across the 117 of their papers we have counts for

collaborators
Showing 2002Show all

10 papers · 1 filter

astro-ph2002★ 56 cited

Highly-Ionized Gas in the Galactic Halo: A FUSE Survey of O VI Absorption toward 22 Halo Stars

J. Zsargo, K. R. Sembach, J. C. Howk +1

Far Ultraviolet Spectroscopic Explorer spectra of 22 Galactic halo stars are studied to determine the amount of O VI in the Galactic halo between ~0.3 and \~10 kpc from the Galacti…

astro-ph2002★ 39 cited

Ionized Gas in the First 10 kpc of the Interstellar Galactic Halo

J. Christopher Howk, Kenneth R. Sembach, Blair D. Savage

We present FUSE observations of the post-asymptotic giant branch star von Zeipel 1128 (l=42.5, b=+78.7; z=10.0 kpc), located in the globular cluster Messier 3. The FUSE observation…

astro-ph2002★ 68 cited

A FUSE Survey of Molecular Hydrogen in Intermediate-Velocity Clouds in the Milky Way Halo

P. Richter, B. P. Wakker, B. D. Savage +1

Far Ultraviolet Spectroscopic Explorer (FUSE) data is used to investigate the molecular hydrogen (H_2) content of intermediate-velocity clouds (IVCs) in the lower halo of the Milky…

astro-ph2002★ 22 cited

Origins of the Highly Ionized Gas along the Line of Sight towards HD 116852

Andrew J. Fox, Blair D. Savage, Kenneth R. Sembach +5

We present Hubble Space Telescope Imaging Spectrograph (HST/STIS) and Far Ultraviolet Spectroscopic Explorer (FUSE) observations of high ion interstellar absorption along the sight…

astro-ph2002

Probing Baryons in Galactic Halos and Gas Near Galaxies

K. R. Sembach, B. P. Wakker, B. D. Savage +2

We describe an extensive FUSE survey of highly ionized oxygen in the vicinity of the Milky Way that serves as an example of the type of study that would be desirable for other gala…

astro-ph2002★ 203 cited

Distribution and Kinematics of O VI in the Galactic Halo

B. D. Savage, K. R. Sembach, B. P. Wakker +6

FUSE spectra of 100 extragalactic objects are analyzed to obtain measures of O VI absorption along paths through the Milky Way thick disk/halo. Strong O VI absorption over the appr…