The End of the MACHO Era: Limits on Halo Dark Matter from Stellar Halo Wide Binaries

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© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Jaiyul Yoo et al 2004 ApJ 601 311 DOI 10.1086/380562

0004-637X/601/1/311

Abstract

We simulate the evolution of halo wide binaries in the presence of the massive compact halo objects (MACHOs) and compare our results to the sample of wide binaries in a companion paper. The observed distribution is well fitted by a single power law for angular separations, 3farcs5 < Δθ < 900'', whereas the simulated distributions show a break in the power law whose location depends on the MACHO mass and density. This allows us to place upper limits on the density of MACHOs as a function of their assumed mass. At the 95% confidence level, we exclude MACHOs with masses M > 43 M at the standard local halo density ρH. This all but removes the last permitted window for a full MACHO halo for masses M > 10-7.5 M.

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10.1086/380562