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Title:
Tidal Tails and the Shape of the Dark Matter Halo
Authors:
Lewis, Geraint F.; Ibata, Rodrigo A.
Affiliation:
AA(School of Physics, University of Sydney, Sydney NSW 2006, Australia ), AB(Observatoire de Strasbourg, 6700 Strasbourg, France)
Publication:
Publications of the Astronomical Society of Australia, Volume 22, Issue 3, pp. 190-194. (PASA Homepage)
Publication Date:
00/2005
Origin:
PASA
Astronomy Keywords:
cosmology: theory, dark matter, galaxies: halos, Galaxy: formation, halo
DOI:
10.1071/AS04080
Bibliographic Code:
2005PASA...22..190L

Abstract

Cold dark matter cosmologies successfully accounts for the distribution of matter on large scales. On smaller scales, these cosmological models predict that galaxies like our own Milky Way should be enveloped in massive dark matter halos. Furthermore, these halos should be significantly flattened or even triaxial. Recent observational evidence, drawn from the demise of the Sagittarius dwarf galaxy as it is cannibalized by our own, indicates that the potential of the Milky Way must be close to spherical. While the precise interpretation of the observational evidence is under debate, an apparently spherical halo may signify a pronounced failing of dark matter models, and may even indicate a failure in our fundamental understanding of gravity.
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