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 1998 · astro-phShow all

8 papers · 2 filters

astro-ph1998

Highly Ionized High Velocity Clouds

Kenneth R. Sembach, Blair D. Savage, Limin Lu +1

We have recently used the Hubble Space Telescope to study a pair of high velocity clouds in the direction of Mrk 509 that have unusual ionization properties. They exhibit strong CI…

astro-ph1998

Observational evidence for the accretion of low-metallicity gas onto the Milky Way; metallicity, physical conditions and distance limit for HVC complex C

B. P. Wakker, J. C. Howk, B. D. Savage +5

We present observations of the (field of the) Seyfert galaxy Mark290, which probes the high-velocity cloud (HVC) complex C, one of the largest HVCs. We find that this object has a…

astro-ph1998

The HI fine structure of HVC187 near NGC3783, gas in the leading bridge of the Magellanic System

B. P. Wakker, B. D. Savage, T. A. Oosterloo +1

We present an analysis of high-resolution HI data of one of the cores of HVC187 Wakker & van Woerden 1991), HVC287+22+240. Structure is present down to the lowest-measurable scale…

astro-ph1998★ 59 cited

The Deuterium Abundance at z=0.701 towards QSO 1718+4807

David Tytler, Scott Burles, Limin Lu +3

We present constraints on the deuterium to hydrogen ratio (D/H) in the metal-poor gas cloud at redshift towards QSO 1718+4807. We use new Keck spectra in addition to Hubb…

astro-ph1998★ 96 cited

Highly Ionized High Velocity Clouds: Intergalactic Gas in the Local Group or Distant Gas in the Galactic Halo?

Kenneth R. Sembach, Blair D. Savage, Limin Lu +1

We have recently identified several high velocity (V < -100 km/s) clouds in the directions of Mrk 509 and PKS 2155-304 that have unusual ionization properties. The clouds exhibit s…

astro-ph1998★ 140 cited

The HST Quasar Absorption Line Key Project. XIV. The Evolution of Ly-alpha Absorption Lines in the Redshift Interval 0 to 1.5

Ray J. Weymann, Buell T. Jannuzi, Limin Lu +10

We present an analysis of the evolution of the Ly alpha absorption lines in the redshift interval 0.0 to \sim 1.5 based upon a sample of 987 lines identified in the spectra of 63 Q…