Evidence for Halo Microlensing from a Survey of M31

Details Evidence for Halo Microlensing from a Survey of M31 Evidence for Halo Microlensing from a Survey of M31

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..220..121c&link_type=abstract

International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the final microlensing result from one survey
(VATT/Columbia) monitoring stars in M31, and the initial results of a
larger study (MEGA), which together seem to indicate the presence of a
microlensing halo component comprising a significant fraction of the
dark matter in M31.

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