The Baryon Halo of the Milky Way: A fossil record of its formation

Joss Bland-Hawthorn*, Ken Freeman

*Corresponding author for this work

    Research output: Contribution to journalReview articlepeer-review

    20 Citations (Scopus)

    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 languageEnglish
    Pages (from-to)79-84
    Number of pages6
    JournalScience
    Volume287
    Issue number5450
    DOIs
    Publication statusPublished - 2000

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