期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 386, 期 4, 页码 2209-2220出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2008.13186.x
关键词
galaxies : abundances; intergalactic medium; quasars : absorption lines; quasars : general
Damped Lyman alpha systems (DLAs) and sub-DLAs seen towards background quasars provide the most detailed probes of elemental abundances. Somewhat paradoxically these measurements are more difficult at lower redshifts due to the atmospheric cut-off, and so a few years ago our group began a program to study abundances at z < 1.5 in quasar absorbers. In this paper, we present new Ultraviolet and Visual Echelle Spectrograph (UVES) observations of six additional quasar absorption-line systems at z < 1.5, five of which are sub-DLAs. We find solar or above solar metallicity, as measured by the abundance of zinc, assumed not to be affected by dust, in two sub-DLAs: one, towards Q0138-0005 with [Zn/H] = +0.28 +/- 0.16 ; the other towards Q2335+1501 with [Zn/H] = +0.07 +/- 0.34 . Relatively high metallicity was observed in another system: Q0123-0058 with [Zn/H] = -0.45 +/- 0.20 . Only for the one DLA in our sample, in Q0449-1645, do we find a low metallicity, [Zn/H] = -0.96 +/- 0.08 . We also note that in some of these systems large relative abundance variations from component to component are observed in Si, Mn, Cr and Zn.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据