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MACHOs: The Plot Thickens

Michael S. Turner·Evalyn I. Gates·Geza Gyuk
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Abstract

We discuss the implications of the recent upward revision of the LMC microlensing rate by the MACHO Collaboration. We conclude: (i) A good case for the existence of baryonic dark matter in the halo has been made; (ii) The case for the existence of cold dark matter is unaffected and still compelling; and (iii) The Galactic halo is still an excellent place to search for cold dark matter particles (e.g., axions or neutralinos).

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Michael S. Turner, Evalyn I. Gates, Geza Gyuk. 1996-01-29. MACHOs: The Plot Thickens. https://arxiv.org/abs/astro-ph/9601168

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