QSO 2359-1241: A bright, highly polarized, radio-moderate, reddened, low-ionization broad absorption line quasar

被引:29
作者
Brotherton, MS
Arav, N
Becker, RH
Tran, HD
Gregg, MD
White, RL
Laurent-Muehleisen, SA
Hack, W
机构
[1] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA
[2] Kitt Peak Natl Observ, Natl Opt Astron Observ, Tucson, AZ 85726 USA
[3] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[4] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[5] Space Telescope Sci Inst, Baltimore, MD 21218 USA
关键词
galaxies : evolution; galaxies : interactions; quasars : emission lines; quasars : general; quasars : individual (QSO J2359-1241);
D O I
10.1086/318243
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a bright quasar (E = 15.8, z = 0.868) associated with the flat-spectrum radio source NVSS J235953 - 124148. This quasar, which we designate QSO 2359 - 1241, possesses a rare combination of extreme properties that make it of special interest. These properties include intrinsic high-velocity outflow seen in absorption for both high- and low-ionization species, high optical polarization (similar to5%), significant radio emission, and dust reddening. The dereddened absolute magnitude of QSO 2359 - 1241 places it among the three most optically luminous quasars known at z < 1. High-resolution spectroscopy and a detailed analysis of the optical/ultraviolet absorption features will be given in a companion paper.
引用
收藏
页码:134 / 139
页数:6
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