University of Hertfordshire

From the same journal

From the same journal

By the same authors

21-cm H I emission from the Damped Lyman-alpha absorber SBS 1543 593

Research output: Contribution to journalArticle

Documents

  • D.V. Bowen
  • W. Huchtmeier
  • E. Brinks
  • T.M. Tripp
  • E.B. Jenkins
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Original languageEnglish
Pages (from-to)820-823
JournalAstronomy and Astrophysics
Journal publication dateJun 2001
Volume372
DOIs
Publication statusPublished - Jun 2001

Abstract

We detect 21-cm emission from the Low Surface Brightness (LSB) galaxy SBS 1543+593, which gives rise to a Damped-Ly (DLy ) absorption line in the spectrum of the background QSO HS 1543+5921 (ze = 0:807). We obtain an accurate measure of the velocity of the H I gas in the LSB galaxy, v = 2868 km s−1, and derive a mass of MHI = 1:3 109 M . We compare MH I with limits obtained towards two other z 0:1 DLy systems, and show that SBS 1543+593 would not have been detected. Hence LSB galaxies similar to SBS 1543+593 can be responsible for DLy systems at even modest redshifts without being detectable from their 21-cm emission.

Notes

Original article can be found at: http://www.aanda.org/--Copyright The European Southern Observatory DOI : 10.1051/0004-6361:20010592

ID: 175762