The baryon halo of the Milky Way: A fossil record of its formation

被引:20
作者
Bland-Hawthorn, J
Freeman, K
机构
[1] Anglo Australian Observ, Epping, NSW 2121, Australia
[2] Australian Natl Univ, Mt Stromlo & Siding Spring Observ, Weston, ACT 2611, Australia
关键词
D O I
10.1126/science.287.5450.79
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Astronomers believe that the baryon (stellar) halo of the Milky Way retains a fossil imprint of how it was formed. But a vast Literature shows that the struggle to interpret the observations within a consistent framework continues. The evidence indicates that the halo has built up through a process of accretion and merging over billions of years, which is still going on at a Low Level. Future satellite missions to derive three-dimensional space motions and heavy element (metal) abundances for a billion stars will disentangle the existing web and elucidate how galaxies Like our own came into existence.
引用
收藏
页码:79 / 84
页数:8
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