Metals and dust in intermediate-redshift damped Lyα galaxies

Pushpa Khare*, Varsha P. Kulkarni, James T. Lauroesch, Donald G. York, Arlin P.S. Crotts, Osamu Nakamura

*この研究の対応する著者

研究成果: Article査読

68 被引用数 (Scopus)

抄録

We report on spectroscopic observations with the Multiple Mirror Telescope for 11 damped Lyα absorbers (DLAs) or strong DLA candidates at 0.1 < z < 1.5, including several absorbers discovered in the Sloan Digital Sky Survey. In particular, we have measured absorption lines of Zn II, Cr II, Ni II, Fe II, Mn II, Ti II, Ca II, and Si II. These measurements have doubled the sample of Zn and Cr measurements at z < 1. The average relative abundance patterns in these objects are very similar to those found for high-redshift DLAs reported in the literature. Our observations suggest that the dust content, as determined by [Cr/Zn], does not show much change with redshift. We also examine the sample for correlation of [Cr/Zn] with estimates of the quasar reddening. Our data suggest that the global mean metallicity of DLAs, as measured by the gas-phase abundance of Zn, at best shows a weak evolution with redshift over the range 0.4 < z < 3.9.

本文言語English
ページ(範囲)86-109
ページ数24
ジャーナルAstrophysical Journal
616
1 I
DOI
出版ステータスPublished - 2004 11月 20
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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