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

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Showing 2004Show all

7 papers · 1 filter

astro-ph2004★ 29 cited

FUSE Observations of Interstellar and Intergalactic Absorption Toward the X-ray Bright BL Lac Object Mrk 421

B. D. Savage, B. P. Wakker, A. J. Fox +1

High-quality Far-Ultraviolet Spectroscopic Explorer (FUSE) observations at 20 km /s resolution of interstellar and intergalactic absorption from 910 to 1187 A are presented for the…

astro-ph2004★ 1 cited

Searching for the Missing Baryons in the Warm-hot Intergalactic Medium

P. Richter, B. D. Savage, T. M. Tripp +1

We discuss physical properties and the baryonic content of the Warm-hot Intergalactic Medium (WHIM) at low redshifts. Cosmological simulations predict that the WHIM contains a larg…

astro-ph2004

Exploring Hot Gas in the Galactic Halo and High Velocity Clouds

Kenneth R. Sembach, Bart P. Wakker, Blair D. Savage +1

In the five years since its launch, the Far Ultraviolet Spectroscopic Explorer has given the astronomical community a marvelous glimpse into the realm of previously unexplored regi…

astro-ph2004

High-velocity OVI in and near the Milky Way

Bart P. Wakker, Blair. D. Savage, Kenneth R. Sembach +2

The Far Ultraviolet Spectroscopic Explorer (FUSE) has observed over three hundred fifty sightlines to extragalactic targets. About one hundred fifty of these are of sufficient qual…

astro-ph2004★ 115 cited

Physical Properties and Baryonic Content of Low-Redshift Intergalactic Ly-alpha and O VI Absorption Systems: The PG1116+215 Sight Line

Kenneth R. Sembach, Todd M. Tripp, Blair D. Savage +1

We present HST and FUSE observations of the intergalactic absorption toward PG1116+215 in the 900-3000 A spectral region. We detect 25 Ly-alpha absorbers at rest-frame equivalent w…

astro-ph2004★ 50 cited

C II Radiative Cooling of the Diffuse Gas in the Milky Way

N. Lehner, B. P. Wakker, B. D. Savage

The heating and cooling of the interstellar medium allow the gas in the ISM to coexist at very different temperatures in thermal pressure equilibrium. The heating cannot be directl…