Constraints on the mass of the dark halo from the rotation curve of the Galaxy

被引：0
|
作者：
Lépine, JRD [1 ]
Amaral, LH [1 ]
机构：
[1] Univ Sao Paulo, Dept Astron, Sao Paulo, Brazil
来源：
THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO | 1999年 / 165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：
We derive upper limits to the amount of dark matter in the Galaxy 1) from the fact that the rotation curve of the Galaxy is declining at large radii, and 2) by comparing mass estimations derived from the rotation curve and from star-counts.
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页码：337 / 340
页数：4
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