activity
19992014
most citedA FUSE Survey of Interstellar Molecular Hydrogen in Translucent Clouds

322 citations · 711 across the 5 of their papers we have counts for

collaborators

6 papers

physics.ao-ph2014

An Astronomer's View of Climate Change

Donald C. Morton

This paper describes some of the astronomical effects that could be important for understanding the ice ages, historic climate changes and the recent temperature increase. These in…

astro-ph2003★ 78 cited

High-Resolution Observations of Interstellar Ca I Absorption -- Implications for Depletions and Electron Densities in Diffuse Clouds

Daniel E. Welty, L. M. Hobbs, Donald C. Morton

We present high-resolution (FWHM ~ 0.3-1.5 km/s) spectra of interstellar Ca I absorption toward 30 Galactic stars. Comparisons of the column densities of Ca I, Ca II, K I, and othe…

astro-ph2002★ 322 cited

A FUSE Survey of Interstellar Molecular Hydrogen in Translucent Clouds

Brian L. Rachford, Theodore P. Snow, Jason Tumlinson +12

We report the first ensemble results from the FUSE survey of molecular hydrogen in lines of sight with A_V 1 mag. We have developed techniques for fitting computed profil…

astro-ph2001★ 132 cited

Resolving the Structure of Ionized Helium in the Intergalactic Medium with the Far Ultraviolet Spectroscopic Explorer

G. A. Kriss, J. M. Shull, W. Oegerle +16

The neutral hydrogen and the ionized helium absorption in the spectra of quasars are unique probes of structure in the early universe. We present Far-Ultraviolet Spectroscopic Expl…

astro-ph2000

Far-UV FUSE spectroscopy of the OVI resonance doublet in Sand2 (WO)

Paul A. Crowther, A. W. Fullerton, D. J. Hillier +10

We present Far-Ultraviolet Spectroscopic Explorer (FUSE) spectroscopy of Sand 2, a LMC WO-type Wolf-Rayet star, revealing the OVI resonance P Cygni doublet at 1032-38A. These data…

astro-ph1999★ 179 cited

The Diffuse Interstellar Clouds toward 23 Orionis

D. E. Welty, L. M. Hobbs, J. T. Lauroesch +3

Spectra obtained with the Hubble Space Telescope GHRS are combined with high-resolution optical spectra and UV spectra from Copernicus to study the abundances and physical conditio…