Diffuse Baryonic Dark Matter in the Galactic Halo

Details Diffuse Baryonic Dark Matter in the Galactic Halo Diffuse Baryonic Dark Matter in the Galactic Halo

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003idm..conf..159j&link_type=abstract

THE IDENTIFICATION OF DARK MATTER. Proceedings of the Fourth International Workshop. Held 2 - 6 September 2002 in York, UK. Edit

Astronomy and Astrophysics

Astrophysics

Baryonic Dark Matter, Galactic Halo

Scientific paper

The nature of the dark matter in the halo of our Galaxy is still largely unknown. The microlensing events found so far towards the Large Magellanic Cloud suggest that at most 20% of the halo dark matter is in the form of MACHOs (Massive Astrophysical Compact Halo Objects) and that they probably belong to different intervening populations. The halo dark matter could also, at least partially, consist of cold molecular clouds (mainly H2).

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