The Tully-Fisher Relation in Numerical Simulations of Structure Formation

被引：0
|
作者：
De Rossi, Maria E. [1 ]
Tissera, Patricia B. [1 ]
Pedrosa, Susana E. [1 ]
机构：
[1] CONICET UBA, Inst Astron & Fis Espacio, RA-1428 Buenos Aires, DF, Argentina
来源：
STELLAR POPULATIONS: PLANNING FOR THE NEXT DECADE | 2010年 / 262期
关键词：
Galaxies: formation; Galaxies: evolution; Cosmology: dark matter; GALAXIES;
D O I：
10.1017/S1743921310003078
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Tully-Fisher Relation (TFR) is of fundamental importance for galaxy formation as it provides information about the relation between the baryonic content of galaxies and the depth of their dark halos potential wells. In recent years, it has been possible to study this relation at different redshifts. However, there are still controversies about its origin and evolution. In this work, we try to address the origin of the Tully-Fisher Relation by employing cosmological hydrodynamical simulations.
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收藏
页码：327 / 328
页数：2
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