The central dark mass of the Milky Way

Details The central dark mass of the Milky Way The central dark mass of the Milky Way

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205...20e&link_type=abstract

Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at

Computer Science

Scientific paper

High resolution infrared imaging and spectroscopy have given in the past five years very valuable new information on the properties and dynamics of the central star cluster of the Milky Way. A review is given what these observations tell us about character and evolution of the cluster, and in particular about the stellar dynamics. It is shown that the measured stellar radial and proper motions make a very strong case for a two to three million solar mass central black hole associated with the compact radio source SgrA*.

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