Recent observations of microlensing events towards the Magellanic Clouds suggest an important fraction of the galactic dark matter may be in the form of MACHOs with mass about 0.1 solar masses. We outline a scenario in which dark clusters of MACHOs and molecular clouds naturally form in the galactic halo and outline possible signatures of this model.
MACHOs and Molecular Clouds in Galactic Halo
DE PAOLIS, Francesco;INGROSSO, Gabriele;
1995-01-01
Abstract
Recent observations of microlensing events towards the Magellanic Clouds suggest an important fraction of the galactic dark matter may be in the form of MACHOs with mass about 0.1 solar masses. We outline a scenario in which dark clusters of MACHOs and molecular clouds naturally form in the galactic halo and outline possible signatures of this model.File in questo prodotto:
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