The gaseous extent of galaxies and the origin of Lyman alpha absorption systems. IV: Lyman alpha absorbers arising in a galaxy group
arXiv:astro-ph/9904232 · doi:10.1086/307719
Abstract
We present new GHRS observations of Lyman alpha absorption lines associated with a group of galaxies towards the QSO 1545+2101. We have identified eight distinct Lyman alpha absorption features in the spectrum of QSO 1545+2101 at a mean redshift of z=0.2648 with a velocity dispersion of 163 km/s. A group of galaxies is detected in the vicinity of this QSO at a mean redshift of z=0.2645 and velocity dispersion 239 km/s. The identification of discrete absorption systems indicates that they arise in clouds of neutral hydrogen rather than in a diffuse intragroup medium. Our analysis suggests that the Lyman alpha absorption lines are associated with individual galaxies in the group, although a one-to-one relationship between absorbers and galaxies is difficult to establish in such a dense environment.
16 pages, 3 figures. Accepted for publication in ApJ
Cited by in corpus (9)
- The Population of Weak MgII Absorbers. II The Properties of Single-Cloud Systems
- Lyman-alpha absorption around nearby galaxies
- A Uniform Analysis of the Ly-alpha Forest at z=0 - 5: V. The extragalactic ionizing background at low redshift
- Warm Gas in the Virgo Cluster: I. Distribution of Lya Absorbers
- Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
- On the Interaction Between Cosmic Rays and Dark Matter Molecular Clouds in the Milky Way. l Basic Considerations
- The association between gas and galaxies I: CFHT spectroscopy and pair analysis
- The Origin of \lya Absorption Systems at ---Implications from the Hubble Deep Field
- Where are the absorbers towards Q2302+029?