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 [J].

Chiba, M ;

Yoshii, Y .

ASTRONOMICAL JOURNAL, 1998, 115 (01) :168-192

[4]

CHIBA M, 1999, UNPUB AJ

[5] EVIDENCE FROM MOTIONS OF OLD STARS THAT GALAXY COLLAPSED [J].

EGGEN, OJ ;

LYNDENBELL, D ;

SANDAGE, AR .

ASTROPHYSICAL JOURNAL, 1962, 136 (03) :748-&

[6] COMPOSITIONS OF HALO CLUSTERS AND FORMATION OF GALACTIC HALO [J].

SEARLE, L ;

ZINN, R .

ASTROPHYSICAL JOURNAL, 1978, 225 (02) :357-379

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