Numerical simulations of the galaxy formation

被引：2

作者：

Bekki, K ^{[1
]}

Chiba, M ^{[1
]}

机构：

[1] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan

来源：

FIRST STARS | 2000年

关键词：

D O I：

10.1007/10719504_38

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We numerically investigate whether the CDM model can reproduce reasonably well chemical, kinematical, and structural properties of the Galactic stellar halo.

引用

页码：206 / 207

页数：2

共 6 条

[1] BEERS TC, 1999, UNPUB AJ
[2] BEKKI K, 1999, UNPUB
[3] Early evolution of the galactic halo revealed from Hipparcos observations of metal-poor stars
Chiba, M
Yoshii, Y
[J]. ASTRONOMICAL JOURNAL, 1998, 115 (01) : 168 - 192
[4] CHIBA M, 1999, UNPUB AJ
[5] EVIDENCE FROM MOTIONS OF OLD STARS THAT GALAXY COLLAPSED
EGGEN, OJ
LYNDENBELL, D
SANDAGE, AR
[J]. ASTROPHYSICAL JOURNAL, 1962, 136 (03) : 748 - &
[6] COMPOSITIONS OF HALO CLUSTERS AND FORMATION OF GALACTIC HALO
SEARLE, L
ZINN, R
[J]. ASTROPHYSICAL JOURNAL, 1978, 225 (02) : 357 - 379

← 1 →