The nature of the ultraluminous X-ray sources inside galaxies and their relation to local QSOs

被引：12

作者：

Burbidge, G ^{[1
]}

Burbidge, EM

Arp, H

机构：

[1] Univ Calif San Diego, Ctr Astrophys & Space Sci 0424, La Jolla, CA 92093 USA

[2] Max Planck Inst Astrophys, D-85741 Garching, Germany

来源：

ASTRONOMY & ASTROPHYSICS | 2003年 / 400卷 / 02期

关键词：

galaxies : active; quasars : general; X-rays : galaxies; X-rays : stars;

D O I：

10.1051/0004-6361:20030134

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is suggested that many of the ultraluminous compact X-ray sources now being found in the main bodies of galaxies, particularly those that are active, like M 82, NGC 3628 and others, are "local" QSOs, or BL Lac objects, with high intrinsic redshifts in the process of being ejected from those galaxies. Evidence bearing on this hypothesis is summarized.

引用

页码：L17 / L19

页数：3

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