activity
19972025
most citedThe COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-Redshift Circumgalactic Medium

573 citations · 8.6k across the 120 of their papers we have counts for

collaborators
Showing 2005Show all

11 papers · 1 filter

astro-ph2005★ 47 cited

High Metallicity, Photoionised Gas in Intergalactic Large-Scale Filaments

Bastien Aracil, Todd M. Tripp, David V. Bowen +3

We present high-resolution UV spectra of absorption-line systems toward the low-z QSO HS0624+6907 (z=0.3700). Coupled with spectroscopic galaxy redshifts, we find that many of thes…

astro-ph2005★ 14 cited

The Deuterium, Oxygen, and Nitrogen Abundance Toward LSE 44

S. D. Friedman, G. Hebrard, T. M. Tripp +2

We present measurements of the column densities of interstellar DI, OI, NI, and H2 made with FUSE, and of HI made with IUE toward the sdO star LSE 44, at a distance of 554+/-66 pc.…

astro-ph2005★ 11 cited

The Connections between QSO Absorption Systems and Galaxies: Low-Redshift Observations

Todd M. Tripp, David V. Bowen

Quasar absorption lines have long been recognized to be a sensitive probe of the abundances, physical conditions, and kinematics of gas in a wide variety of environments including…

astro-ph2005★ 37 cited

Measurements of the f-Values of the Resonance Transitions of Ni II at 1317.217A and 1370.132A

Edward B. Jenkins, Todd M. Tripp

We have retrieved high-resolution UV spectra of 69 hot stars from the HST archive and determined the strengths of the interstellar Ni II absorption features at 1317.217A. We then c…

astro-ph2005★ 66 cited

Tracing baryons in the warm-hot intergalactic medium with broad Ly alpha absorption

Philipp Richter, Blair Savage, Ken Sembach +1

We discuss physical properties and baryonic content of broad Ly alpha absorbers (BLAs) at low redshift. These absorption systems, recently discovered in high-resolution, high-signa…

astro-ph2005★ 50 cited

A Comparison of Absorption and Emission Line Abundances in the Nearby Damped Lyman-alpha Galaxy SBS 1543+593

David V. Bowen, Edward B. Jenkins, Max Pettini +1

We have used the Space Telescope Imaging Spectrograph (STIS) aboard HST to measure a sulfur abundance of [S/H] = -0.41 +/-0.06 in the interstellar medium (ISM) of the nearby damped…