ZWICKY-3146 - THE MOST MASSIVE COOLING FLOW

被引：32

作者：

EDGE, AC ^{[1
]}

FABIAN, AC ^{[1
]}

ALLEN, SW ^{[1
]}

CRAWFORD, CS ^{[1
]}

WHITE, DA ^{[1
]}

BOHRINGER, H ^{[1
]}

VOGES, W ^{[1
]}

机构：

[1] MAX PLANCK INST EXTRATERR PHYS,D-85740 GARCHING,GERMANY

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 270卷 / 01期

关键词：

GALAXIES; CLUSTERING; CLUSTERS; INDIVIDUAL; ZW-3146; COOLING FLOWS; X-RAYS;

D O I：

10.1093/mnras/270.1.L1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this Letter we present a deep ROSAT HRI image of Zwicky 3146 (or Zw 37-19), a distant cluster with high X-ray luminosity. The X-ray data show that the cluster contains the most massive known cooling flow at 1250 M. yr-1, the existence of which has important implications for the formation and evolution of the cluster. The central galaxy in the cluster shows strong optical line emission and a blue continuum, and is also aligned with the X-ray emission.

引用

页码：L1 / L5

页数：5

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