THE STRUCTURE OF THE BAL QSO-1700+518

被引：18

作者：

HUTCHINGS, JB

NEFF, SG

GOWER, AC

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771

[2] UNIV VICTORIA,DEPT PHYS & ASTRON,VICTORIA V8W 2Y2,BC,CANADA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1992年 / 104卷 / 671期

关键词：

D O I：

10.1086/132958

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present 0.5 arcsec resolution optical images of the low-redshift, bright, broad-absorption-line (BAL) QSO 1700 + 518. We find a bright arc 2 arcsec to the NE of the nucleus which is redder than the surrounding host galaxy. There is also a faint radial structure to the SE, which is aligned with the core radio structure. The principal radio structure is a slightly resolved component coincident with the optical nucleus and an unresolved lobe 1 arcsec to the W which has no corresponding optical structure. We discuss the morphological and other properties of the QSO.

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页码：62 / 65

页数：4

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