M31 - A unique laboratory for gravitational microlensing

Details M31 - A unique laboratory for gravitational microlensing M31 - A unique laboratory for gravitational microlensing

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...399l..43c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 399, no. 1, p. L43-L46.

Statistics

Computation

158

Galactic Bulge, Gravitational Lenses, Halos, Milky Way Galaxy, Computational Astrophysics, Galactic Structure

Scientific paper

Due to the smaller angular size of its stars, its greater mass, and the
favorable geometry of its nearly edge-on disk, M31 offers interesting
advantages in the search for gravitational microlensing by massive
condensed halo objects (MACHOs). These advantages and the techniques
which can be used to exploit them are discussed here.

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