Abstract
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.
Original language | English |
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Pages (from-to) | 79-84 |
Number of pages | 6 |
Journal | Science |
Volume | 287 |
Issue number | 5450 |
DOIs | |
Publication status | Published - 2000 |