Recent observations of microlensing events in the LMC suggest that a sizable fraction of the galactic halo is in the form of MACHOs. We describe a scenario in which dark clusters of MACHOs and cold molecular clouds naturally form at galactocentric distances larger than 10-20 kpc.
MACHOs as Brown Dwarfs
DE PAOLIS, Francesco;INGROSSO, Gabriele;
1998-01-01
Abstract
Recent observations of microlensing events in the LMC suggest that a sizable fraction of the galactic halo is in the form of MACHOs. We describe a scenario in which dark clusters of MACHOs and cold molecular clouds naturally form at galactocentric distances larger than 10-20 kpc.File in questo prodotto:
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