MACHOs and molecular clouds in galaxies.

Details MACHOs and molecular clouds in galaxies. MACHOs and molecular clouds in galaxies.

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ncimb.112..295d&link_type=abstract

Nuovo Cimento B, Vol. 112B, No. 2 - 3, p. 295 - 298

Astronomy and Astrophysics

Astrophysics

1

Gravitational Microlensing: Galactic Halo, Gravitational Microlensing: Galactic Halos, Gravitational Microlensing: Magellanic Clouds, Gravitational Microlensing: Andromeda Galaxy

Scientific paper

Observations of microlensing events towards the Magellanic Clouds suggest that an important fraction of the Galactic halo is in the form of massive astrophysical compact halo objects (MACHOs) with mass ≡0.1 Msun. The authors propose a model for the formation of dark clusters of MACHOs and molecular clouds in the galactic halo at distances larger than ≡10 - 20 kpc from the center. Possible signatures of the presence of molecular clouds in our Galaxy and in M31 are considered.

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