QSO Absorption Line Constraints on Intragroup High-Velocity Clouds
arXiv:astro-ph/0002001 · doi:10.1086/317265
Abstract
We show that the number statistics of moderate redshift MgII and Lyman limit absorbers may rule out the hypothesis that high velocity clouds are infalling intragroup material.
4 pages, no figures; submitted to Astrophysical Journal Letters; revised version, more general and includes more about Braun and Burton CHVCs
References in corpus (2)
Cited by in corpus (19)
- Highly-Ionized High-Velocity Gas in the Vicinity of the Galaxy
- Complex C: A Low-Metallicity High-Velocity Cloud Plunging into the Milky Way
- New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?
- The Population of Weak MgII Absorbers. II The Properties of Single-Cloud Systems
- High-velocity clouds as streams of ionized and neutral gas in the halo of the Milky Way
- A Survey of FUSE and HST Sightlines through High-Velocity Cloud Complex C
- A Hubble Space Telescope Study of Lyman Limit Systems: Census and Evolution
- The abundance of dark galaxies
- A Very Sensitive 21cm Survey for Galactic High-Velocity HI
- A Targeted Survey for HI Clouds in Galaxy Groups
- CaII and NaI absorption signatures from extraplanar gas in the halo of the Milky Way
- Where are the High Velocity Clouds in Local Group Analogs?
- Cold gas accretion by high-velocity clouds and their connection to QSO absorption-line systems
- An absorption-selected survey of neutral gas in the Milky Way halo
- A Limit on the Metallicity of Compact High Velocity Clouds
- Low Redshift QSO Lyman alpha Absorption Line Systems Associated with Galaxies
- High Velocity Cloud Edges and Mini-HVCs
- The HI Detection of Low Column Density Clouds and Galaxies
- On the origin of gaseous galaxy halos - Low-column density gas in the Milky Way halo