B0850+054: a new gravitational lens system from CLASS

被引:15
作者
Biggs, AD [1 ]
Rusin, D
Browne, IWA
de Bruyn, AG
Jackson, NJ
Koopmans, LVE
McKean, JP
Myers, ST
Blandford, RD
Chae, KH
Fassnacht, CD
Norbury, MA
Pearson, TJ
Phillips, PM
Readhead, ACS
Wilkinson, PN
机构
[1] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] Joint Inst VLBI Europe, NL-7990 AA Dwingeloo, Netherlands
[3] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[4] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[5] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[6] ASTRON, NL-7990 AA Dwingeloo, Netherlands
[7] CALTECH, Pasadena, CA 91125 USA
[8] Natl Radio Astron Observ, Socorro, NM 87801 USA
[9] Space Telescope Sci Inst, Baltimore, MD 21218 USA
关键词
gravitational lensing; quasars : individual : B0850+054;
D O I
10.1046/j.1365-8711.2003.06159.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a new gravitational lens system from the CLASS survey. Radio observations with the VLA, WSRT and MERLIN show that the radio source B0850+054 is composed of two compact components with identical spectra, a separation of 0.7 arcsec and a flux density ratio of 6 : 1. VLBA observations at 5 GHz reveal structures that are consistent with the gravitational lens hypothesis. The brighter of the two images is resolved into a linear string of at least six subcomponents, whilst the weaker image is radially stretched towards the lens galaxy. UKIRT K -band imaging detects an 18.7-mag extended object, but the resolution of the observations is not sufficient to resolve the lensed images and the lens galaxy. Mass modelling has not been possible with the present data and the acquisition of high-resolution optical data is a priority for this system.
引用
收藏
页码:1084 / 1088
页数:5
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