Intergalactic HeII absorption towards QSO 1157+3143

被引:41
作者
Reimers, D
Fechner, C
Hagen, HJ
Jakobsen, P
Tytler, D
Kirkman, D
机构
[1] Univ Hamburg, Hamburger Sternwarte, D-21029 Hamburg, Germany
[2] European Space Agcy, Estec, RSSD, Astrophys Missions Div, NL-2200 AG Noordwijk, Netherlands
[3] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
来源
ASTRONOMY & ASTROPHYSICS | 2005年 / 442卷 / 01期
关键词
galaxies : quasars : individual : QSO 1157+3143; galaxies : quasars : absorption lines; cosmology : observations;
D O I
10.1051/0004-6361:20053365
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a further line of sight allowing detection of He II Ly alpha absorption by the intergalactic medium. A HST/STIS survey of 32 bright z similar to 3 quasars selected from the Hamburg Quasar Surveys yielded one detection toward QSO 1157+3143 ( z similar to 3, B similar or equal to 17). A 10 orbit follow-up spectrum reveals a UV spectrum significantly suppressed by two intervening Lyman limit systems at z = 2.77 and 2.94, but with the continuum flux recovering sufficiently shortward of similar to 1700 angstrom to allow study of the He II absorption spectrum in the redshift range 2.75 <= z <= 2.97. The absorption is characterized by alternating voids and dense filament structures seen in both He II and H I. Attempts to model the He II opacity in terms of H I Ly alpha forest absorption are not successful in the voids, suggesting that He II reionization is not complete between z = 2.77 and 2.97 or that an optically thin Lyman limit system with z approximate to 0.3 is responsible for the additional opacity.
引用
收藏
页码:63 / 68
页数:6
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