The complex gravitational lens system B1933+503

被引:54
作者
Sykes, CM [1 ]
Browne, IWA
Jackson, NJ
Marlow, DR
Nair, S
Wilkinson, PN
Blandford, RD
Cohen, J
Fassnacht, CD
Hogg, D
Pearson, TJ
Readhead, ACS
Womble, DS
Myers, ST
de Bruyn, AG
Bremer, M
Miley, GK
Schilizzi, RT
机构
[1] Univ Manchester, Nuffield Radio Astron Labs, Jodrell Bank, Macclesfield SK11 9DL, Cheshire, England
[2] CALTECH, Pasadena, CA 91125 USA
[3] Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[4] Joint Inst VLBI Europe, NL-7990 AA Dwingeloo, Netherlands
[5] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[6] Kapteyn Lab, NL-9700 AA Groningen, Netherlands
关键词
gravitation; galaxies : active; galaxies : individual : B1933+503; gravitational lensing; radio continuum : galaxies;
D O I
10.1046/j.1365-8711.1998.02081.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of the most complex arcsec-scale radio gravitational lens system yet known, B1933+503 was found during the course of the CLASS survey and MERLIN and VLA radio maps reveal up to 10 components. Four of these are compact and have flat spectra: the rest are more extended and have steep spectra, The background lensed object appears to consist of a flat-spectrum core (quadruply imaged) and two compact 'lobes' symmetrically disposed relative to the core, One of the lobes is quadruply imaged while the other is doubly imaged. An HST observation of the system with the WFPC2 shows a galaxy with an axial ratio of 0.5, but none of the images of the background object is detected, A redshift of 0.755 has been measured for the lens galaxy.
引用
收藏
页码:310 / 314
页数:5
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