The Baryon Halo of the Milky Way: A Fossil Record of Its Formation
Joss Bland-Hawthorn,
1
Ken Freeman
2
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.
1 Anglo-Australian Observatory, PO Box 296, Epping,
NSW 2121, Australia.
2 Mount Stromlo and Siding Spring
Observatories, Private Bag, Weston Creek ACT 2611, Australia.
To whom correspondence should be addressed: E-mail:
jbh{at}aaoepp.aao.gov.au