An illuminating dark halo

Stéphane Colombi
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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

Nature, 2008, vol. 456, issue 7218, 44-45

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.

Date: 2008
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DOI: 10.1038/456044a

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