Unveiling the powerful quasar hidden in the nucleus of the FR II radio galaxy 3C 265

被引：2

作者：

Bondi, M

Brunetti, G

Comastri, A

Setti, G

机构：

[1] CNR, Ist Radioastron, I-40129 Bologna, Italy

[2] INAF, Osservatorio Astron Bologna, Bologna, Italy

[3] Univ Bologna, Dipartimento Astron, Bologna, Italy

来源：

NEW ASTRONOMY REVIEWS | 2003年 / 47卷 / 6-7期

关键词：

galaxies : active; galaxies : individual : 3C 265: X-ray: galaxies; radio continuum : galaxies; radiation mechanism : non-thermal;

D O I：

10.1016/S1387-6473(03)00068-X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The radio source 3C 265, located at z = 0.811, is one of the most luminous radio galaxies in the 3CR catalogue. Indirect evidence for the presence of a powerful quasar in the nucleus of 3C 265 was provided by optical, infrared, and radio studies. We present preliminary results from new Chandra X-ray observations of the radio galaxy 3C 265, allowing us to test the presence of such a powerful quasar, and at the same time to study the effect of the intense nuclear flux on the relativistic electron population in the radio lobes of 3C 265. (C) 2003 Elsevier B.V. All rights reserved.

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收藏

页码：443 / 445

页数：3

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