The great disk of Milky-Way satellites and cosmological sub-structures

被引：314

作者：

Kroupa, P ^{[1
]}

Theis, C

Boily, CM

机构：

[1] Univ Kiel, Inst Theoret Phys & Astrophys, D-24098 Kiel, Germany

[2] Sternwarte Bonn, D-53121 Bonn, Germany

[3] Univ Vienna, Inst Astron, A-1180 Vienna, Austria

[4] Observ Astron, F-67000 Strasbourg, France

来源：

ASTRONOMY & ASTROPHYSICS | 2005年 / 431卷 / 02期

关键词：

Galaxy : evolution; Galaxy : halo; galaxies : dwarf; galaxies : kinematics and dynamics; galaxies : Local Group; Galaxy : formation;

D O I：

10.1051/0004-6361:20041122

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that the shape of the observed distribution of Milky Way ( MW) satellites is inconsistent with their being drawn from a cosmological sub-structure population with a confidence of 99.5 per cent. Most of the MW satellites therefore cannot be related to dark-matter dominated satellites.

引用

页码：517 / 521

页数：5

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