Dark matter haloes in isolated interacting galaxy pairs

被引：0

作者：

Fuentes-Carrera, I ^{[1
]}

Rosado, M ^{[1
]}

Amram, P ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico

来源：

GALAXY EVOLUTION: THEORY AND OBSERVATIONS | 2003年 / 17卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

SMost of the studies attempting to characterise the mass-to-luminosity ratio (M/L) and the structure of dark matter haloes in isolated interacting galaxy pairs have used a statistical approach of the, problem. It is important though to restrain these parameters through the detailed observations and analysis of,the kinematics and dynamics of specific interacting galaxy pairs. We present results on the preliminary study of the M-51 type interacting galaxy pair Kar302 (NGC 3893/96).

引用

页码：44 / 44

页数：1

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