RADIO STRUCTURE OF 3C123 AT 2.7 AND 15GHZ

被引：26

作者：

RILEY, JM

POOLEY, GG

机构：

[1] Mullard Radio Astronomy Observatory, Cavendish Laboratory, Madingley Road, CBS, Cambridge,OHE, United Kingdom

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1978年 / 183卷 / 01期

关键词：

D O I：

10.1093/mnras/183.2.245

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

3C123 has been mapped at 2.7 and 15 GHz with resolutions 3.6 x 7.2 and 0.65 x 1.3 arcsec, in total power and polarization. A compact central source, coincident with the optical galaxy, has been discovered. The polarization data suggest the presence of large amounts of 'cold' matter within the components. © Royal Astronomical Society.

引用

页码：245 / 255

页数：11

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