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

117 papers

astro-ph.GA2024★ 2 cited

A Search for 3-mm Molecular Absorption Line Transitions in the Magellanic Stream

Lucille Steffes, Daniel R. Rybarczyk, Snežana Stanimirović +14

The Magellanic Stream, a tidal tail of diffuse gas falling onto the Milky Way, formed by interactions between the Small and Large Magellanic Clouds, is primarily composed of neutra…

astro-ph.GA2023★ 19 cited

The Distribution of Metallicities in the Local Galactic Interstellar Medium

Adam M. Ritchey, Edward B. Jenkins, J. Michael Shull +3

In this investigation, we present an analysis of the metallicity distribution that pertains to neutral gas in the local Galactic interstellar medium (ISM). We derive relative ISM m…

astro-ph.GA2021★ 20 cited

Molecular Gas within the Milky Way's Nuclear Wind

Frances H. Cashman, Andrew J. Fox, Blair D. Savage +9

We report the first direct detection of molecular hydrogen associated with the Galactic nuclear wind. The Far-Ultraviolet Spectroscopic Explorer spectrum of LS 4825, a B1 Ib-II sta…

astro-ph.GA2021★ 15 cited

The HI Column Density Distribution of the Galactic Disk and Halo

David M. French, Andrew J. Fox, Bart P. Wakker +8

We present a census of neutral gas in the Milky Way disk and halo down to limiting column densities of (HI) cm using measurements of HI Lyman-series absorpti…

astro-ph.GA2021★ 16 cited

The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems

Aditya Manuwal, Anand Narayanan, Purvi Udhwani +4

We present here results from a survey of intervening C IV absorbers at conducted using 223 sightlines from the Hubble Spectroscopic Legacy Archive. Most systems (83%) ou…

astro-ph.CO2020★ 18 cited

The evolution of the low-density HI intergalactic medium from z=3.6 to 0: Data, transmitted flux and HI column density

Tae-Sun Kim, Bart P. Wakker, Fahad Nasir +8

We present a new, uniform analysis of the HI transmitted flux (F) and HI column density (N(HI)) distribution in the low-density IGM as a function of redshift z for 0<z<3.6 using 55…