Skip to main navigation Skip to search Skip to main content

The gaseous extent of galaxies and the origin of Lyα absorption systems. IV. Lyα absorbers arising in a galaxy group

  • A. Ortiz-Gil
  • , K. M. Lanzetta
  • , J. K. Webb
  • , X. Barcons
  • , A. Fernández-Soto
  • Stony Brook University
  • University of New South Wales
  • Consejo Superior de Investigaciones Cientificas - Universidad de Cantabria

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

We present new Goddard High Resolution Spectrograph observations of Lyα absorption lines associated with a group of galaxies toward the QSO 1545 + 2101. We have identified eight distinct Lyα 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-1. A group of galaxies is detected in the vicinity of this QSO at a mean redshift of 〈z〉 = 0.2645 and velocity dispersion of 239 km s-1. 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 Lyα 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.

Original languageEnglish
Pages (from-to)72-77
Number of pages6
JournalAstrophysical Journal
Volume523
Issue number1 PART 1
DOIs
StatePublished - Sep 20 1999

Keywords

  • Galaxies: ISM
  • Quasars: absorption lines

Fingerprint

Dive into the research topics of 'The gaseous extent of galaxies and the origin of Lyα absorption systems. IV. Lyα absorbers arising in a galaxy group'. Together they form a unique fingerprint.

Cite this