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An illuminating dark halo

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  • Stéphane Colombi

    (Stéphane Colombi is at the Institut d'Astrophysique de Paris, CNRS UMR 7095/Université Pierre et Marie Curie, 98 bis boulevard Arago, 75014 Paris, France. colombi@iap.fr)

Abstract

A large simulation reveals that most of the detectable signal from dark matter in our Milky Way probably comes from the main, smooth Galactic halo, rather than from small clumps.

Suggested Citation

  • Stéphane Colombi, 2008. "An illuminating dark halo," Nature, Nature, vol. 456(7218), pages 44-45, November.
    • Handle: RePEc:nat:nature:v:456:y:2008:i:7218:d:10.1038_456044a
    DOI: 10.1038/456044a
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