15 research outputs found
The stellar halo of the Galaxy
Stellar halos may hold some of the best preserved fossils of the formation
history of galaxies. They are a natural product of the merging processes that
probably take place during the assembly of a galaxy, and hence may well be the
most ubiquitous component of galaxies, independently of their Hubble type. This
review focuses on our current understanding of the spatial structure, the
kinematics and chemistry of halo stars in the Milky Way. In recent years, we
have experienced a change in paradigm thanks to the discovery of large amounts
of substructure, especially in the outer halo. I discuss the implications of
the currently available observational constraints and fold them into several
possible formation scenarios. Unraveling the formation of the Galactic halo
will be possible in the near future through a combination of large wide field
photometric and spectroscopic surveys, and especially in the era of Gaia.Comment: 46 pages, 16 figures. References updated and some minor changes.
Full-resolution version available at
http://www.astro.rug.nl/~ahelmi/stellar-halo-review.pd
Reconstructing Galaxy Histories from Globular Clusters
Nearly a century after the true nature of galaxies as distant "island
universes" was established, their origin and evolution remain great unsolved
problems of modern astrophysics. One of the most promising ways to investigate
galaxy formation is to study the ubiquitous globular star clusters that
surround most galaxies. Recent advances in our understanding of the globular
cluster systems of the Milky Way and other galaxies point to a complex picture
of galaxy genesis driven by cannibalism, collisions, bursts of star formation
and other tumultuous events.Comment: Review Article published in Nature, 1 January 2004. 18 pages, 4
figures, pdf format onl