J. Christopher Howk
0000-0002-2591-3792
University of Notre Dame
111 papers found
Refreshing results…
The Hidden Mass and Large Spatial Extent of a Post-Starburst Galaxy Outflow
A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way
Ahubble Space Telescopestudy of Lyman Limit Systems: Census and Evolution
The Interstellar Medium and Star Formation in Edge-On Galaxies. I. Ngc 891
Fundamental Properties of the Highly Ionized Plasmas in the Milky Way
Origin(s) of the Highly Ionized High-Velocity Clouds Based on Their Distances
Wavelength Accuracy of the Keck Hires Spectrograph and Measuring Changes in the Fine Structure Constant
Properties and Origin of the High-Velocity Gas Toward the Large Magellanic Cloud
Strong z ∼ 0.5 O vi absorption towards PKS 0405−123: implications for ionization and metallicity of the Cosmic Web★
The CONNECTION BETWEEN a LYMAN LIMIT SYSTEM, a VERY STRONG O VI ABSORBER, AND GALAXIES ATz∼ 0.203
Probing feedback in protogalaxies: multiphase gas in a DLA atz≈ 2.4
The High‐Velocity Gas toward Messier 5: Tracing Feedback Flows in the Inner Galaxy
Metallicity and Physical Conditions in the Magellanic Bridge1
Simulating anisotropic thermal conduction in supernova remnants – I. Numerical methods
Simulating anisotropic thermal conduction in supernova remnants – II. Implications for the interstellar medium
Distances to Galactic High‐Velocity Clouds. I. Cohen Stream, Complex GCP, Cloud g1
Distances to Galactic High-Velocity Clouds: Complex C
The UCSD/Keck Damped Lyα Abundance Database: A Decade of High‐Resolution Spectroscopy
Highly ionized plasma in the Large Magellanic Cloud: evidence for outflows and a possible galactic wind
Strongly Variable z = 1.48 Fe ii and Mg ii Absorption in the Spectra of z = 4.05 GRB 060206
Missing publications? Search for publications with a matching author name.